The interface between the Earth's surface and outer space. The Kármán line at an altitude of 100 km (62 mi) is shown. The layers of the atmosphere are drawn to scale, whereas objects within them, such as the International Space Station, are not.
Outer space, or just space, is the expanse that exists beyond the Earth and between celestial bodies. Outer space is not completely empty—it is a hard vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium, as well as electromagnetic radiation, magnetic fields, neutrinos, dust, and cosmic rays. The baseline temperature, as set by the background radiation from the Big Bang, is 2.7 kelvins (−270.45 °C; −454.81 °F). The plasma between galaxies accounts for about half of the baryonic (ordinary) matter in the universe; it has a number density of less than one hydrogen atom per cubic metre and a temperature of millions of kelvins; local concentrations of this plasma have condensed into stars and galaxies. Studies indicate that 90% of the mass in most galaxies is in an unknown form, called dark matter, which interacts with other matter through gravitational but not electromagnetic forces. Observations suggest that the majority of the mass-energy in the observable universe is a poorly understood vacuum energy of space, which astronomers label dark energy. Intergalactic space takes up most of the volume of the universe, but even galaxies and star systems consist almost entirely of empty space.
The concept of a Universe filled with a luminiferous aether retained support among some scientists until the early 20th century. This form of aether was viewed as the medium through which light could propagate. In 1887, the Michelson–Morley experiment tried to detect the Earth's motion through this medium by looking for changes in the speed of light depending on the direction of the planet's motion. However, the null result indicated something was wrong with the concept. The idea of the luminiferous aether was then abandoned. It was replaced by Albert Einstein's theory of special relativity, which holds that the speed of light in a vacuum is a fixed constant, independent of the observer's motion or frame of reference.
The modern concept of outer space is based on the "Big Bang" cosmology, first proposed in 1931 by the Belgian physicist Georges Lemaître. This theory holds that the universe originated from a very dense form that has since undergone continuous expansion.
The earliest known estimate of the temperature of outer space was by the Swiss physicist Charles É. Guillaume in 1896. Using the estimated radiation of the background stars, he concluded that space must be heated to a temperature of 5–6 K. British physicist Arthur Eddington made a similar calculation to derive a temperature of 3.18 K in 1926. German physicist Erich Regener used the total measured energy of cosmic rays to estimate an intergalactic temperature of 2.8 K in 1933. American physicists Ralph Alpher and Robert Herman predicted 5 K for the temperature of space in 1948, based on the gradual decrease in background energy following the then-new Big Bang theory. The modern measurement of the cosmic microwave background is about 2.7K.
This is an artist's concept of the metric expansion of space, where a volume of the Universe is represented at each time interval by the circular sections. At left is depicted the rapid inflation from the initial state, followed thereafter by steady expansion to the present day, shown at right.
Part of the Hubble Ultra-Deep Field image showing a typical section of space containing galaxies interspersed by deep vacuum. Given the finite speed of light, this view covers the past 13 billion years of the history of outer space.
Because of the hazards of a vacuum, astronauts must wear a pressurized space suit while off-Earth and outside their spacecraft.
SpaceShipOne completed the first manned private spaceflight in 2004, reaching an altitude of 100.12 km (62.21 mi).
The Outer Space Treaty provides the basic framework for international space law. It covers the legal use of outer space by nation states, and includes in its definition of outer space the Moon and other celestial bodies. The treaty states that outer space is free for all nation states to explore and is not subject to claims of national sovereignty. It also prohibits the deployment of nuclear weapons in outer space. The treaty was passed by the United Nations General Assembly in 1963 and signed in 1967 by the USSR, the United States of America and the United Kingdom. As of 2017, 105 state parties have either ratified or acceded to the treaty. An additional 25 states signed the treaty, without ratifying it.
Since 1958, outer space has been the subject of multiple United Nations resolutions. Of these, more than 50 have been concerning the international co-operation in the peaceful uses of outer space and preventing an arms race in space. Four additional space law treaties have been negotiated and drafted by the UN's Committee on the Peaceful Uses of Outer Space. Still, there remains no legal prohibition against deploying conventional weapons in space, and anti-satellite weapons have been successfully tested by the US, USSR, China, and in 2019, India The 1979 Moon Treaty turned the jurisdiction of all heavenly bodies (including the orbits around such bodies) over to the international community. However, this treaty has not been ratified by any nation that currently practices manned spaceflight.
Geospace is the region of outer space near Earth, including the upper atmosphere and magnetosphere. The Van Allen radiation belts lie within the geospace. The outer boundary of geospace is the magnetopause, which forms an interface between the Earth's magnetosphere and the solar wind. The inner boundary is the ionosphere. The variable space-weather conditions of geospace are affected by the behavior of the Sun and the solar wind; the subject of geospace is interlinked with heliophysics—the study of the Sun and its impact on the planets of the Solar System.
The day-side magnetopause is compressed by solar-wind pressure—the subsolar distance from the center of the Earth is typically 10 Earth radii. On the night side, the solar wind stretches the magnetosphere to form a magnetotail that sometimes extends out to more than 100–200 Earth radii. For roughly four days of each month, the lunar surface is shielded from the solar wind as the Moon passes through the magnetotail.
Interplanetary space is defined by the solar wind, a continuous stream of charged particles emanating from the Sun that creates a very tenuous atmosphere (the heliosphere) for billions of kilometers into space. This wind has a particle density of 5–10 protons/cm3 and is moving at a velocity of 350–400 km/s (780,000–890,000 mph). Interplanetary space extends out to the heliopause where the influence of the galactic environment starts to dominate over the magnetic field and particle flux from the Sun. The distance and strength of the heliopause varies depending on the activity level of the solar wind. The heliopause in turn deflects away low-energy galactic cosmic rays, with this modulation effect peaking during solar maximum.
The deep vacuum of space could make it an attractive environment for certain industrial processes, such as those requiring ultraclean surfaces. However, like asteroid mining, space manufacturing requires significant investment with little prospect of immediate return. An important factor in the total expense is the high cost of placing mass into Earth orbit: $7,000–25,000 per kg in inflation-adjusted dollars, according to a 2006 estimate. Proposed concepts for addressing this issue include non-rocket spacelaunch, momentum exchange tethers, and space elevators.
^ Chuss, David T. (June 26, 2008), Cosmic Background Explorer, NASA Goddard Space Flight Center, archived from the original on May 9, 2013, retrieved 2013-04-27.
^ a b Gupta, Anjali; Galeazzi, M.; Ursino, E. (May 2010), "Detection and Characterization of the Warm-Hot Intergalactic Medium", Bulletin of the American Astronomical Society, 41: 908, Bibcode:2010AAS...21631808G.
^ Freedman & Kaufmann 2005, pp. 573, 599–601.
^ Trimble, V. (1987), "Existence and nature of dark matter in the universe", Annual Review of Astronomy and Astrophysics, 25: 425–472, Bibcode:1987ARA&A..25..425T, doi:10.1146/annurev.aa.25.090187.002233.
^ "Dark Energy, Dark Matter", NASA Science, archived from the original on June 2, 2013, retrieved May 31, 2013, It turns out that roughly 68% of the Universe is dark energy. Dark matter makes up about 27%.
^ Freedman & Kaufmann 2005, pp. 650–653.
^ a b O'Leary 2009, p. 84.
^ a b "Where does space begin? – Aerospace Engineering, Aviation News, Salary, Jobs and Museums". Aerospace Engineering, Aviation News, Salary, Jobs and Museums. Archived from the original on 2015-11-17. Retrieved 2015-11-10.
^ Grant 1981, p. 10.
^ Porter, Park & Daston 2006, p. 27.
^ Eckert 2006, p. 5.
^ Needham & Ronan 1985, pp. 82–87.
^ Holton & Brush 2001, pp. 267–268.
^ Cajori 1917, pp. 64–66.
^ Genz 2001, pp. 127–128.
^ Tassoul & Tassoul 2004, p. 22.
^ Gatti 2002, pp. 99–104.
^ Kelly 1965, pp. 97–107.
^ Olenick, Apostol & Goodstein 1986, p. 356.
^ Hariharan 2003, p. 2.
^ Olenick, Apostol & Goodstein 1986, pp. 357–365.
^ Thagard 1992, pp. 206–209.
^ Maor 1991, p. 195.
^ Webb 1999, pp. 71–73.
^ Curtis, Heber D. (January 1988), "Novae in Spiral Nebulae and the Island Universe Theory", Publications of the Astronomical Society of the Pacific, 100: 6–7, Bibcode:1988PASP..100....6C, doi:10.1086/132128.
^ Cepheid Variable Stars & Distance Determination, CSIRO Australia, October 25, 2004, archived from the original on August 30, 2011, retrieved 2011-09-12.
^ Tyson & Goldsmith 2004, pp. 114–115.
^ Lemaître, G. (May 1931), "The Beginning of the World from the Point of View of Quantum Theory", Nature, 127 (3210): 706, Bibcode:1931Natur.127..706L, doi:10.1038/127706b0.
^ a b Assis, A. K. T.; Paulo, São; Neves, M. C. D. (July 1995), "History of the 2.7 K Temperature Prior to Penzias and Wilson", Apeiron, 2 (3): 79–87.
^ Stuart Wortley 1841, p. 410.
^ Von Humboldt 1845, p. 39.
^ Harper, Douglas, "Outer", Online Etymology Dictionary, archived from the original on 2010-03-12, retrieved 2008-03-24.
^ Harper, Douglas (November 2001), Space, The Online Etymology Dictionary, archived from the original on 2009-02-24, retrieved 2009-06-19.
^ Planck Collaboration (2014), "Planck 2013 results. I. Overview of products and scientific results", Astronomy & Astrophysics, 571: 1, arXiv:1303.5062, Bibcode:2014A&A...571A...1P, doi:10.1051/0004-6361/201321529.
^ a b Turner, Michael S. (September 2009), "Origin of the Universe", Scientific American, 301 (3): 36–43, Bibcode:2009SciAm.301c..36T, doi:10.1038/scientificamerican0909-36, PMID 19708526.
^ Silk 2000, pp. 105–308.
^ WMAP – Shape of the universe, NASA, December 21, 2012, archived from the original on June 1, 2012, retrieved June 4, 2013.
^ Sparke & Gallagher 2007, pp. 329–330.
^ Wollack, Edward J. (June 24, 2011), What is the Universe Made Of?, NASA, archived from the original on July 26, 2016, retrieved 2011-10-14.
^ Krumm, N.; Brosch, N. (October 1984), "Neutral hydrogen in cosmic voids", Astronomical Journal, 89: 1461–1463, Bibcode:1984AJ.....89.1461K, doi:10.1086/113647.
^ Peebles, P.; Ratra, B. (2003). "The cosmological constant and dark energy". Reviews of Modern Physics. 75 (2): 559–606. arXiv:astro-ph/0207347. Bibcode:2003RvMP...75..559P. doi:10.1103/RevModPhys.75.559.
^ Tadokoro, M. (1968), "A Study of the Local Group by Use of the Virial Theorem", Publications of the Astronomical Society of Japan, 20: 230, Bibcode:1968PASJ...20..230T. This source estimates a density of 7 × 10−29 g/cm3 for the Local Group. An atomic mass unit is 1.66 × 10−24 g, for roughly 40 atoms per cubic meter.
^ Borowitz & Beiser 1971.
^ Tyson, Patrick (January 2012), The Kinetic Atmosphere: Molecular Numbers (PDF), archived from the original (PDF) on 16 March 2014, retrieved 13 September 2013.
^ Davies 1977, p. 93.
^ Fitzpatrick, E. L. (May 2004), "Interstellar Extinction in the Milky Way Galaxy", in Witt, Adolf N.; Clayton, Geoffrey C.; Draine, Bruce T., Astrophysics of Dust, ASP Conference Series, 309, p. 33, arXiv:astro-ph/0401344, Bibcode:2004ASPC..309...33F.
^ Chamberlain 1978, p. 2.
^ Squire, Tom (September 27, 2000), "U.S. Standard Atmosphere, 1976", Thermal Protection Systems Expert and Material Properties Database, NASA, archived from the original on October 15, 2011, retrieved 2011-10-23.
^ Forbes, Jeffrey M. (2007), "Dynamics of the thermosphere" (PDF), Journal of the Meteorological Society of Japan, Series II, 85B: 193–213, doi:10.2151/jmsj.85b.193, archived from the original (PDF) on 2012-04-15, retrieved 2012-03-25.
^ a b Prialnik 2000, pp. 195–196.
^ Spitzer 1978, p. 28–30.
^ Chiaki, Yanagisawa (June 2014), "Looking for Cosmic Neutrino Background", Frontiers in Physics, 2: 30, Bibcode:2014FrP.....2...30Y, doi:10.3389/fphy.2014.00030.
^ Fixsen, D. J. (December 2009), "The Temperature of the Cosmic Microwave Background", The Astrophysical Journal, 707 (2): 916–920, arXiv:0911.1955, Bibcode:2009ApJ...707..916F, doi:10.1088/0004-637X/707/2/916.
^ Withbroe, George L. (February 1988), "The temperature structure, mass, and energy flow in the corona and inner solar wind", Astrophysical Journal, Part 1, 325: 442–467, Bibcode:1988ApJ...325..442W, doi:10.1086/166015.
^ Wielebinski, Richard; Beck, Rainer (2010), "Cosmic Magnetic Fields − An Overview", in Block, David L.; Freeman, Kenneth C.; Puerari, Ivânio, Galaxies and their Masks: A Conference in Honour of K.C. Freeman, FRS, Springer Science & Business Media, pp. 67–82, Bibcode:2010gama.conf...67W, doi:10.1007/978-1-4419-7317-7_5, ISBN 978-1441973177, archived from the original on 2017-09-20.
^ Letessier-Selvon, Antoine; Stanev, Todor (July 2011), "Ultrahigh energy cosmic rays", Reviews of Modern Physics, 83 (3): 907–942, arXiv:1103.0031, Bibcode:2011RvMP...83..907L, doi:10.1103/RevModPhys.83.907.
^ Lang 1999, p. 462.
^ Lide 1993, p. 11-217.
^ What Does Space Smell Like?, Live Science, July 20, 2012, archived from the original on February 28, 2014, retrieved February 19, 2014.
^ Lizzie Schiffman (July 17, 2013), What Does Space Smell Like, Popular Science, archived from the original on February 24, 2014, retrieved February 19, 2014.
^ Raggio, J.; et al. (May 2011), "Whole Lichen Thalli Survive Exposure to Space Conditions: Results of Lithopanspermia Experiment with Aspicilia fruticulosa", Astrobiology, 11 (4): 281–292, Bibcode:2011AsBio..11..281R, doi:10.1089/ast.2010.0588, PMID 21545267.
^ Tepfer, David; et al. (May 2012), "Survival of Plant Seeds, Their UV Screens, and nptII DNA for 18 Months Outside the International Space Station" (PDF), Astrobiology, 12 (5): 517–528, Bibcode:2012AsBio..12..517T, doi:10.1089/ast.2011.0744, PMID 22680697, archived (PDF) from the original on 2014-12-13, retrieved 2013-05-19.
^ Wassmann, Marko; et al. (May 2012), "Survival of Spores of the UV-ResistantBacillus subtilis Strain MW01 After Exposure to Low-Earth Orbit and Simulated Martian Conditions: Data from the Space Experiment ADAPT on EXPOSE-E", Astrobiology, 12 (5): 498–507, Bibcode:2012AsBio..12..498W, doi:10.1089/ast.2011.0772, PMID 22680695.
^ Nicholson, W. L. (April 2010), "Towards a General Theory of Lithopanspermia", Astrobiology Science Conference 2010, 1538, pp. 5272–528, Bibcode:2010LPICo1538.5272N.
^ Piantadosi 2003, pp. 188–189.
^ a b Bolonkin, Alexander (2009), "Man in Outer Space Without a Special Space Suit", American Journal of Engineering and Applied Sciences, 2 (4): 573–579, doi:10.3844/ajeassp.2009.573.579, archived from the original on 2017-08-29, retrieved 2011-12-15.
^ Krebs, Matthew B.; Pilmanis, Andrew A. (November 1996), Human pulmonary tolerance to dynamic over-pressure, United States Air Force Armstrong Laboratory, archived from the original on 2012-11-30, retrieved 2011-12-23.
^ Harding, R. M.; Mills, F. J. (April 30, 1983), "Aviation medicine. Problems of altitude I: hypoxia and hyperventilation", British Medical Journal, 286 (6375): 1408–1410, doi:10.1136/bmj.286.6375.1408, PMC 1547870.
^ Hodkinson, P. D. (March 2011), "Acute exposure to altitude" (PDF), Journal of the Royal Army Medical Corps, 157 (1): 85–91, doi:10.1136/jramc-157-01-15, PMID 21465917, archived from the original (PDF) on 2012-02-20, retrieved 2011-12-16.
^ Billings 1973, pp. 1–34.
^ Landis, Geoffrey A. (August 7, 2007), Human Exposure to Vacuum, www.geoffreylandis.com, archived from the original on July 21, 2009, retrieved 2009-06-19.
^ Webb, P. (1968), "The Space Activity Suit: An Elastic Leotard for Extravehicular Activity", Aerospace Medicine, 39 (4): 376–383, PMID 4872696.
^ Ellery 2000, p. 68.
^ Davis, Johnson & Stepanek 2008, pp. 270–271.
^ Kanas, Nick; Manzey, Dietrich (2008), "Basic Issues of Human Adaptation to Space Flight", Space Psychology and Psychiatry, Space Technology Library, 22: 15–48, Bibcode:2008spp..book.....K, doi:10.1007/978-1-4020-6770-9_2, ISBN 978-1-4020-6769-3.
^ Williams, David; et al. (June 23, 2009), "Acclimation during space flight: effects on human physiology", Canadian Medical Association Journal, 180 (13): 1317–1323, doi:10.1503/cmaj.090628, PMC 2696527, PMID 19509005.
^ Kennedy, Ann R., Radiation Effects, National Space Biological Research Institute, archived from the original on 2012-01-03, retrieved 2011-12-16.
^ Setlow, Richard B. (November 2003), "The hazards of space travel", Science and Society, 4 (11): 1013–1016, doi:10.1038/sj.embor.7400016, PMC 1326386, PMID 14593437.
^ Michael Coren (July 14, 2004), "Private craft soars into space, history", CNN.com, archived from the original on April 2, 2015.
^ Wong & Fergusson 2010, p. 16.
^ Petty, John Ira (February 13, 2003), "Entry", Human Spaceflight, NASA, archived from the original on October 27, 2011, retrieved 2011-12-16.
^ Thompson, Andrea (April 9, 2009), Edge of Space Found, space.com, archived from the original on July 14, 2009, retrieved 2009-06-19.
^ Sangalli, L.; et al. (2009), "Rocket-based measurements of ion velocity, neutral wind, and electric field in the collisional transition region of the auroral ionosphere", Journal of Geophysical Research, 114 (A4): A04306, Bibcode:2009JGRA..114.4306S, doi:10.1029/2008JA013757.
^ Status of International Agreements relating to activities in outer space as of 1 January 2017 (PDF), United Nations Office for Outer Space Affairs/ Committee on the Peaceful Uses of Outer Space, March 23, 2017, archived from the original (PDF) on March 22, 2018, retrieved 2018-03-22.
^ Treaty on Principles Governing the Activities of States in the Exploration and Use of Outer Space, including the Moon and Other Celestial Bodies, United Nations Office for Outer Space Affairs, January 1, 2008, archived from the original on February 22, 2011, retrieved 2009-12-30.
^ Index of Online General Assembly Resolutions Relating to Outer Space, United Nations Office for Outer Space Affairs, 2011, archived from the original on 2010-01-15, retrieved 2009-12-30.
^ Wong & Fergusson 2010, p. 4.
^ Solanki, Lalit (2019-03-27). "India Enters the Elite Club: Successfully Shot Down Low Orbit Satellite". The Mirk. Retrieved 2019-03-28.
^ Columbus launch puts space law to the test, European Science Foundation, November 5, 2007, archived from the original on December 15, 2008, retrieved 2009-12-30.
^ Representatives of the States traversed by the Equator (December 3, 1976), "Declaration of the first meeting of equatorial countries", Space Law, Bogota, Republic of Colombia: JAXA, archived from the original on November 24, 2011, retrieved 2011-10-14.
^ Gangale, Thomas (2006), "Who Owns the Geostationary Orbit?", Annals of Air and Space Law, 31, archived from the original on 2011-09-27, retrieved 2011-10-14.
^ Hill, James V. H. (April 1999), "Getting to Low Earth Orbit", Space Future, archived from the original on 2012-03-19, retrieved 2012-03-18.
^ Shiner, Linda (November 1, 2007), X-15 Walkaround, Air & Space Magazine, retrieved 2009-06-19.
^ Dimotakis, P.; et al. (October 1999), 100 lbs to Low Earth Orbit (LEO): Small-Payload Launch Options, The Mitre Corporation, pp. 1–39, archived from the original on 2017-08-29, retrieved 2012-01-21.
^ Ghosh 2000, pp. 47–48.
^ a b Kennewell, John; McDonald, Andrew (2011), Satellite Lifetimes and Solar Activity, Commonwealth of Australia Bureau of Weather, Space Weather Branch, archived from the original on 2011-12-28, retrieved 2011-12-31.
^ Williams, David R. (November 17, 2010), "Earth Fact Sheet", Lunar & Planetary Science, NASA, archived from the original on October 30, 2010, retrieved 2012-05-10.
^ a b Schrijver & Siscoe 2010, p. 363.
^ a b Abby Cessna (July 5, 2009), "Interplanetary space", Universe Today, archived from the original on March 19, 2015.
^ a b Jia-Rui Cook (September 12, 2013), "How do we know when Voyager reaches interstellar space?", JPL News, 2013-278, archived from the original on September 15, 2013.
^ Kintner, Paul; GMDT Committee and Staff (September 2002), Report of the Living With a Star Geospace Mission Definition Team (PDF), NASA, archived (PDF) from the original on 2012-11-02, retrieved 2012-04-15.
^ Fichtner & Liu 2011, pp. 341–345.
^ Koskinen 2010, pp. 32, 42.
^ Mendillo 2000, p. 275.
^ Goodman, John M. (2006). Space Weather & Telecommunications. Springer Science & Business Media. p. 244. ISBN 978-0-387-23671-1.
^ "Geomagnetic Storms" (PDF), OECD/IFP Futures Project on "Future Global Shocks", CENTRA Technology, Inc., pp. 1–69, January 14, 2011, archived (PDF) from the original on March 14, 2012, retrieved 2012-04-07.
^ Portree, David; Loftus, Joseph (1999), Orbital Debris: A Chronology (PDF), NASA, p. 13, archived from the original (PDF) on 2000-09-01, retrieved 2012-05-05.
^ Strickland, John K. (October 1, 2012). "The cislunar gateway with no gate". The Space Review. Archived from the original on February 7, 2016. Retrieved 2016-02-10.
^ Yoder, Charles F. (1995), "Astrometric and Geodetic Properties of Earth and the Solar System", in Ahrens, Thomas J., Global earth physics a handbook of physical constants (PDF), AGU reference shelf Series, 1, Washington, DC: American Geophysical Union, p. 1, Bibcode:1995geph.conf....1Y, ISBN 978-0-87590-851-9, archived from the original (PDF) on April 26, 2012, retrieved 2011-12-31. . This work lists a Hill sphere radius of 234.9 times the mean radius of Earth, or 234.9 × 6,371 km = 1.5 million km.
^ Barbieri 2006, p. 253.
^ Dickson 2010, p. 57.
^ United States, p. 536.
^ Williamson 2006, p. 97.
^ "Definition of 'deep space'", Collins English Dictionary, retrieved 2018-01-15.
^ "ITU-R Radio Regulations, Article 1, Terms and definitions, Section VIII, Technical terms relating to space, paragraph 1.177" (PDF). International Telecommunication Union. Retrieved 2018-02-05.
^ a b Papagiannis 1972, pp. 12–149.
^ Phillips, Tony (2009-09-29), Cosmic Rays Hit Space Age High, NASA, archived from the original on 2009-10-14, retrieved 2009-10-20.
^ Kohler, Susanna (December 1, 2017), "A Shifting Shield Provides Protection Against Cosmic Rays", Nova, American Astronomical Society, retrieved 2019-01-31.
^ NASA (12 March 2019). "What scientists found after sifting through dust in the solar system". EurekAlert!. Retrieved 12 March 2019.
^ Flynn, G. J.; et al. (2003), "The Origin of Organic Matter in the Solar System: Evidence from the Interplanetary Dust Particles", in Norris, R.; Stootman, F., Bioastronomy 2002: Life Among the Stars, Proceedings of IAU Symposium No. 213, 213, p. 275, Bibcode:2004IAUS..213..275F.
^ Leinert, C.; Grun, E. (1990), "Interplanetary Dust", Physics of the Inner Heliosphere I: 207, Bibcode:1990pihl.book..207L.
^ Johnson, R. E. (August 1994), "Plasma-Induced Sputtering of an Atmosphere", Space Science Reviews, 69 (3–4): 215–253, Bibcode:1994SSRv...69..215J, doi:10.1007/BF02101697.
^ a b Ferrière, Katia M. (2001), "The interstellar environment of our galaxy", Reviews of Modern Physics, 73 (4): 1031–1066, arXiv:astro-ph/0106359, Bibcode:2001RvMP...73.1031F, doi:10.1103/RevModPhys.73.1031.
^ Witt, Adolf N. (October 2001), "The Chemical Composition of the Interstellar Medium", Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences – Origin and early evolution of solid matter in the Solar System, 359 (1787), p. 1949, Bibcode:2001RSPTA.359.1949W, doi:10.1098/rsta.2001.0889.
^ Boulares, Ahmed; Cox, Donald P. (December 1990), "Galactic hydrostatic equilibrium with magnetic tension and cosmic-ray diffusion", Astrophysical Journal, Part 1, 365: 544–558, Bibcode:1990ApJ...365..544B, doi:10.1086/169509.
^ Rauchfuss 2008, pp. 72–81.
^ Klemperer, William (August 15, 2006), "Interstellar chemistry", Proceedings of the National Academy of Sciences of the United States of America, 103 (33): 12232–12234, Bibcode:2006PNAS..10312232K, doi:10.1073/pnas.0605352103, PMC 1567863, PMID 16894148.
^ Redfield, S. (September 2006), "The Local Interstellar Medium", New Horizons in Astronomy; Proceedings of the Conference Held 16–18 October 2005 at The University of Texas, Austin, Texas, USA, Frank N. Bash Symposium ASP Conference Series, 352, p. 79, arXiv:astro-ph/0601117, Bibcode:2006ASPC..352...79R.
^ McComas, D. J.; et al. (2012), "The Heliosphere's Interstellar Interaction: No Bow Shock", Science, 336 (6086): 1291–3, Bibcode:2012Sci...336.1291M, doi:10.1126/science.1221054, PMID 22582011.
^ a b Fox, Karen C. (May 10, 2012), NASA – IBEX Reveals a Missing Boundary at the Edge of the Solar System, NASA, archived from the original on May 12, 2012, retrieved 2012-05-14.
^ Wszolek 2013, p. 67.
^ Jafelice, Luiz C.; Opher, Reuven (July 1992), "The origin of intergalactic magnetic fields due to extragalactic jets", Monthly Notices of the Royal Astronomical Society, 257 (1): 135–151, Bibcode:1992MNRAS.257..135J, doi:10.1093/mnras/257.1.135.
^ Wadsley, James W.; et al. (August 20, 2002), "The Universe in Hot Gas", Astronomy Picture of the Day, NASA, archived from the original on June 9, 2009, retrieved 2009-06-19.
^ a b Fang, T.; et al. (2010), "Confirmation of X-Ray Absorption by Warm-Hot Intergalactic Medium in the Sculptor Wall", The Astrophysical Journal, 714 (2): 1715, arXiv:1001.3692, Bibcode:2010ApJ...714.1715F, doi:10.1088/0004-637X/714/2/1715.
^ Bykov, A. M.; Paerels, F. B. S.; Petrosian, V. (February 2008), "Equilibration Processes in the Warm-Hot Intergalactic Medium", Space Science Reviews, 134 (1–4): 141–153, arXiv:0801.1008, Bibcode:2008SSRv..134..141B, doi:10.1007/s11214-008-9309-4.
^ Wakker, B. P.; Savage, B. D. (2009), "The Relationship Between Intergalactic H I/O VI and Nearby (z<0.017) Galaxies", The Astrophysical Journal Supplement Series, 182 (1): 378, arXiv:0903.2259, Bibcode:2009ApJS..182..378W, doi:10.1088/0067-0049/182/1/378.
^ Mathiesen, B. F.; Evrard, A. E. (2001), "Four Measures of the Intracluster Medium Temperature and Their Relation to a Cluster's Dynamical State", The Astrophysical Journal, 546 (1): 100, arXiv:astro-ph/0004309, Bibcode:2001ApJ...546..100M, doi:10.1086/318249.
^ Pfotzer, G. (June 1972), "History of the Use of Balloons in Scientific Experiments", Space Science Reviews, 13 (2): 199–242, Bibcode:1972SSRv...13..199P, doi:10.1007/BF00175313.
^ O'Leary 2009, pp. 209–224.
^ Harrison 2002, pp. 60–63.
^ Hardesty, Eisman & Krushchev 2008, pp. 89–90.
^ Collins 2007, p. 86.
^ Harris 2008, pp. 7, 68–69.
^ Wall, Mike (September 12, 2013), "Voyager 1 Has Left Solar System", Web, Space.com, archived from the original on 14 September 2013, retrieved 13 September 2013.
^ Harrington, J.D.; Villard, Ray; Weaver, Donna (12 December 2012), NASA's Hubble Provides First Census of Galaxies Near Cosmic Dawn, NASA, 12-428, archived from the original on 22 March 2015.
^ Landgraf, M.; et al. (February 2001), "IRSI/Darwin: peering through the interplanetary dust cloud", ESA Bulletin, 105 (105): 60–63, arXiv:astro-ph/0103288, Bibcode:2001ESABu.105...60L.
^ Maccone, Claudio (August 2001), "Searching for bioastronomical signals from the farside of the Moon", in Ehrenfreund, P.; Angerer, O.; Battrick, B., Exo-/astro-biology. Proceedings of the First European Workshop, 496, Noordwijk: ESA Publications Division, pp. 277–280, Bibcode:2001ESASP.496..277M, ISBN 978-92-9092-806-5.
^ Razani 2012, pp. 97–99.
^ Chapmann, Glenn (May 22–27, 1991), "Space: the Ideal Place to Manufacture Microchips", in Blackledge, R.; Radfield, C.; Seida, S., Proceedings of the 10th International Space Development Conference (PDF), San Antonio, Texas, pp. 25–33, archived from the original (PDF) on 2011-07-06, retrieved 2010-01-12.
^ Forgan, Duncan H.; Elvis, Martin (October 2011), "Extrasolar asteroid mining as forensic evidence for extraterrestrial intelligence", International Journal of Astrobiology, 10 (4): 307–313, arXiv:1103.5369, Bibcode:2011IJAsB..10..307F, doi:10.1017/S1473550411000127.
^ Burton, Rodney; Brown, Kevin; Jacobi, Anthony (May 2005), "Low-Cost Launch of Payloads to Low Earth Orbit", Journal of Spacecraft and Rockets, 43 (3): 696–698, Bibcode:2006JSpRo..43..696B, doi:10.2514/1.16244.
^ Bolonkin 2010, p. xv.
^ Crawford, I. A. (September 1990), "Interstellar Travel: A Review for Astronomers", Quarterly Journal of the Royal Astronomical Society, 31: 377–400, Bibcode:1990QJRAS..31..377C.
Borowitz, Sidney; Beiser, Arthur (1971), Essentials of physics: a text for students of science and engineering, Addison-Wesley series in physics (2nd ed.), Addison-Wesley Publishing Company Note: this source gives a value of 2.7 × 1025 molecules per cubic meter.
Davies, P. C. W. (1977), The physics of time asymmetry, University of California Press, ISBN 978-0-520-03247-7 Note: a light year is about 1013 km.
Dickson, Paul (2010), A Dictionary of the Space Age, New Series in NASA History, JHU Press, ISBN 978-0801895043.
Kelly, Suzanne (1965), The de muno of William Gilbert, Amsterdam: Menno Hertzberger & Co.
Stuart Wortley, Emmeline Charlotte E. (1841), The maiden of Moscow, a poem, How and Parsons, Canto X, section XIV, lines 14–15, All Earth in madness moved,—o'erthrown, / To outer space—driven—racked—undone!


text:
package elasticthought

import "github.com/couchbaselabs/logg"

// The logging keys available in elastic thought
var LogKeys []string

func init() {
	LogKeys = []string{
		"CLI",
		"REST",
		"ELASTIC_THOUGHT",
		"MODEL",
		"CLASSIFIER",
		"CHANGES",
		"JOB_SCHEDULER",
		"NSQ_WORKER",
		"DATASET_SPLITTER",
		"DATAFILE_DOWNLOADER",
		"SOLVER",
		"TRAINING_JOB",
		"CLASSIFY_JOB",
		"TEST",
		"CBFS",
	}
}

// Enable logging for all logging keys
func EnableAllLogKeys() {
	for _, logKey := range LogKeys {
		logg.LogKeys[logKey] = true
	}

}

redpajama_set_name: RedPajamaGithub


Kayaking is a water sport which can be both fun and relaxing. Kayaks are canoe-like boats and there are different types including one person kayaks, two people kayaks, inflatable, closed decked kayaks and sit on top kayaks. Kayaking can be enjoyed on river rapids, lakes, waterfalls and even in the sea. The word kayaking means "hunter's boat" and originally they were created by the Inuit, also known as Eskimos.
As a form of exercise, every sport has health benefits associated with them. Kayaking offers a great upper body workout as you paddle through the water. Kayaking is also great for your mental health as it can offer a relaxing and calming experience. Kayaking also is beneficial for your core as you need to use it to hold your balance and turn.
Unfortunately, sometimes the unexpected can happen. Some of the most common injuries associated with kayaking could include a shoulder sprain or strain from pushing the paddle through water, wrist injuries from repetitive movement of the wrist joint, collision injuries and dehydration and sunburn from overexposure of the sun.
Our kayaking sports accident insurance has been designed to provide financial benefit in the case of an injury. Sometimes sporting injuries may mean you are unable to work and our sports accident insurance can help out with the costs associated with that.
Kayaking health insurance is there for you if you occur an injury. Our sports health insurance is designed to give you peace of mind when it comes to looking after your health. You will be able to focus on yourself, your recovery process and returning to doing what you enjoy.
We also offer our private health insurance which is ideal for both individuals and families who are looking at protecting their health. We have over 30 years of experience and are the preferred provider for the Association of Surgeons of Great Britain and Ireland.


text:
Q: How can I join multiple large text files I have about 12,000 .txt files. Most about 10mb in size. I need to join them all into one large text file.  Mostly I use Notepad++ but the "combine" plug doesn't work with it anymore. I've tried a couple freeware options but they freak out over the number and size.  And trying to use the windows command line copy option freaks out, again because there's so many.  I know I could probably do a few at a time or just open each one and copy and paste into a file... but that will take forever.  Is there any other way?!

A: If Notepad++ is not a hard requirement, you could use the COPY command to do this. This will copy the contents of all .txt files to a new file called output:
copy *.txt output

If that does not work for whatever reason, you could try a short script such as this (save as a .bat file in the same folder as the files you want to join):
if exist output del output

for %%a in (*.txt) do (
    type "%%a" >> output
)

A: As @Toto said in comments

If you have a linux machine, you could do: cat *.txt > result.txt

Except that you no longer need a Linux box -  Windows 10 also has a Bash shell, so install it and use the cat command with wildcards to match all  file names to be combined.

redpajama_set_name: RedPajamaStackExchange


"Escuela de arroces y paella Valencia" organises Paella cooking classes. We joint them during our short visit to this exiting city. When we arrived at the restaurant in C. Juristas, coffee was served. Before the cooking could start we first visited the market ( Mercado central) for the ingredients needed. We were in a small international group; Italians, Brazilians and Japanese. We bought the 3 different types of special beans needed for paella.
We walked criss-cross the market and also bought chicken and rabbit meat, tomatoes, rosemary, safran and smoked paprika powder. All ingredients for the paella Valencia.
After returning to the restaurant we got a apron and a togue we started cooking. We cooked Valencian paella with chicken and rabbit. According to the staff the only way to make a good paella!
For the vegetarians a vegetarian paella, which was finished much quicker, was made by the staff.
If you want the recipes, please feel free send us an email.
Offcourse we also eat the paella after starters of mussels, salted tuna and sweet peppers. The funny thing was that the three couples produced a different paella, with the same instructions! Only because a different use if the amount of salt or smoked paprika powder.
The owner served us a nice wine to pair with paella.
Finishing with a crema Valencia, a strong "licor locale" and a "cafe con Leche". It was a great workshop! Although to price is a bit to high if you look at the ingredients used and the type of dish you will make. But very friendly staff and in the end we received a "real Paella diploma"!


We keep on with the theory of "quality first, provider initially, constant improvement and innovation to meet the customers" with the management and "zero defect, zero complaints" as the standard objective. To great our company, we deliver the merchandise using the fantastic excellent at the reasonable price for Cat6 Ftp Keystone Jack , Cat6 FTP Keystone Jack , Cat6 Keystone Jacks , and create an extended term business enterprise romantic relationship with purchasers and users everywhere in the planet.
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text:
Q: Algoritmo para definir prioridade de ordem de serviço Boa noite. Sou iniciante na programação e estudante de T.I. acabei de criar minha conta aqui no Stackoveflow.
Tenho noções básicas (BEM básicas) de Python e JavaScript (e HTML e CSS também).
Estou tentando desenvolver um programa simples para um projeto do meu curso, onde temos uma "empresa" de T.I. que precisa de um método de controle de fluxo de atendimento, para definir a prioridade das ordens de serviço.
A ideia é que o programa faça algumas perguntas referente ao atendimento. Cada pergunta recebe um valor caso a resposta seja positiva ou negativa. Ao final do programa, os valores são somados, e se atingem um determinado score, são categorizados como Prioridade 1, Prioridade 2 ou Prioridade 3.
Fiz um modelo usando JavaScript e HTML, porém, não ta funcionando de jeito nenhum.
Peguem leve, sei que muito provavelmente devem ter alguns erros bem esdrúxulos.
Se alguém puder dar uma força, agradeço

var per1 = document.getElementByName('p1');
var per2 = document.getElementByName('p2');
var per3 = document.getElementByName('p3');
var rs = document.getElementById('res');

function calc() {
  if (per1 == 's') {
    var per1 = 1;
  } else if (per1 == n) {
    var per1 = 2;
  } else {
    alert('Por favor, digite um valor válido!');
  }

  if (per2 == s) {
    var per2 = 1;
  } else if (per2 == n) {
    var per2 = 2;
  } else {
    alert('Por favor, digite um valor válido!');
  }

  if (per3 == s) {
    var per3 = 3;
  } else if (per3 == n) {
    var per3 = 1;
  } else {
    alert('Por favor, digite um valor válido!');
  }
  var rs = (per1 + per2 + per2);
  innerHTML.res += ` ${rs}`;
}
<!doctype html>

  <meta charset=utf-8>
  <title>Priority IT</title>
  <link rel="stylesheet" href="style.css">

Priority IT - dualreceiver

Perguntas:

Responda com "s" para SIM ou "n" NÃO:

1. O diagnóstico foi conciso? <input type="text" name="p1">

2. Você considera que o problema será resolvido de forma relativamente rápida? <input type="text" name="p2">

3. Cliente é PCD, idoso ou necessita atenção especial? <input type="text" name="p3">

    <input type="button" value="Calculate" onclick='calc()'>

 Calculando...

A: *

*Você tem que pegar os valores dos inputs dentro da função, e não fora. Isso porque ao chamar a função, as variáveis às quais são atribuídas os valores dos inputs estarão sempre vazias no carregamento da página, e a função não irá pegar os valores corretos no momento em que a função for chamada.

*document.getElementByName não existe. Existe document.getElementsByName (Elements e não Element). E como document.getElementsByName retorna uma lista de nós, é preciso usar o índice [0], e para pegar o valor do input, acrescentar .value no final: document.getElementsByName('p1')[0].value.

*Faltaram as aspas nas strings s e n dentro dos if's, senão essas letras serão tratadas como variáveis que não existem.

*Já que as variáveis per1, per2 e per3 já foram declaradas com var, não é necessário utilizar var novamente para alterar seus valores.

*innerHTML.res está incorreto. Primeiro vem o elemento e depois o .innerHTML, assim: res.innerHTML.

*Coloque um return após cada alert para impedir que a função chegue até o final em caso de entrar num bloco else.

*Na soma dos valores você repetiu o per2 no final: per1 + per2 + per2, quando o correto seria: per1 + per2 + per3

*No innerHTML não precisaria utilizar o operador +=. Se você quer substituir o conteúdo da div#res, o operador seria apenas o =.

*Colocar uma div dentro de um
 é incorreto no HTML. Você pode utilizar apenas o
, desta forma:
 Calculando...
.

Seu código ficaria assim:

var rs = document.getElementById('res');

function calc() {
   var per1 = document.getElementsByName('p1')[0].value;
   var per2 = document.getElementsByName('p2')[0].value;
   var per3 = document.getElementsByName('p3')[0].value;
  if (per1 == 's') {
    per1 = 1;
  } else if (per1 == 'n') {
    per1 = 2;
  } else {
    alert('Por favor, digite um valor válido!');
    return;
  }

  if (per2 == 's') {
    per2 = 1;
  } else if (per2 == 'n') {
    per2 = 2;
  } else {
    alert('Por favor, digite um valor válido!');
    return;
  }

  if (per3 == 's') {
    per3 = 3;
  } else if (per3 == 'n') {
    per3 = 1;
  } else {
    alert('Por favor, digite um valor válido!');
    return;
  }
  var rs = (per1 + per2 + per3);
  res.innerHTML = ` ${rs}`;
}

Priority IT - dualreceiver

Perguntas:

Responda com "s" para SIM ou "n" NÃO:

1. O diagnóstico foi conciso? <input type="text" name="p1">

2. Você considera que o problema será resolvido de forma relativamente rápida? <input type="text" name="p2">

3. Cliente é PCD, idoso ou necessita atenção especial? <input type="text" name="p3">

   <input type="button" value="Calculate" onclick='calc()'>

 Calculando...


37 relations: Alban MacLellan, Alberta general election, 1935, Alberta general election, 1940, Alberta Liberal Party, Alberta Social Credit Party, Athabasca (provincial electoral district), Calgary (provincial electoral district), Camrose (provincial electoral district), Charles Cathmer Ross, Charles Cockroft, Clarence Tade, Court of Queen's Bench of Alberta, Edmonton (provincial electoral district), Edward Leslie Gray, George Van Allen, Grouard (electoral district), Hans Wight, Innisfail (provincial electoral district), James Hansen (politician), John Hugill, Joseph Tremblay, Leonidas Giroux, Lethbridge (provincial electoral district), Mayo Clinic, Okotoks-High River, Peter M. Campbell, Progressive Conservative Association of Alberta, Samuel A. Barnes, Stettler (provincial electoral district), Stony Plain (electoral district), Taber (provincial electoral district), Walter Morrish, William Aberhart, William Chant, William Hayes (politician), William Morrison (Alberta politician), William R. Howson.
Alban Erskine MacLellan (February 9, 1902 – December 20, 1968) was a railway foreman and a provincial politician from Alberta, Canada.
The Alberta general election of 1935 was the eighth general election for the Province of Alberta, Canada.
The Alberta general election of 1940 was the ninth general election for the Province of Alberta, Canada, was held on March 21, 1940, to elect members of the Legislative Assembly of Alberta.
The Alberta Liberal Party is a provincial political party in Alberta, Canada.
The Alberta Social Credit Party was a provincial political party in Alberta, Canada, that was founded on social credit monetary policy put forward by Clifford Hugh Douglas and on conservative Christian social values.
Athabasca was a provincial electoral district covering north east Alberta, Canada.
Calgary was a provincial electoral district in Alberta, Canada that existed from 1905 to 1913 and was recreated from 1921 to 1959.
Camrose is a provincial electoral district in Alberta, Canada.
Charles Cathmer Ross (June 14, 1884 – September 12, 1938) was a provincial politician from Alberta, Canada.
Charles C. Cockroft (March 20, 1887 – October 16, 1970) was a provincial politician from Alberta, Canada.
Clarence H. Tade (March 15, 1883 – January 5, 1961) was a provincial politician from Alberta, Canada.
The Court of Queen's Bench of Alberta (abbreviated in citations as ABQB or Alta. Q.B.) is the superior court of the Canadian province of Alberta.
The Edmonton provincial electoral district existed in two incarnations from 1905 - 1909 and again from 1921 - 1955, with the city (small as it was in former times) broken up into multiple constituencies in the other time-periods.
Edward Leslie Gray (April 8, 1895 – June 13, 1992) was a politician and member of the Legislative Assembly of Alberta from Alberta, Canada.
George Harold Van Allen (June 22, 1890 – June 15, 1937) was a provincial politician from Alberta, Canada.
Grouard was a provincial electoral district in Alberta, Canada.
Hans Enoch Wight was a provincial politician from Alberta, Canada.
Innisfail is a former Alberta provincial electoral district that existed from 1905 to 1993.
James Hansen (February 17, 1884 – May 14, 1951) was a provincial politician from Alberta, Canada.
John William Hugill (October 3, 1881 – January 13, 1971) was a Canadian lawyer and politician who served as Attorney General of the province of Alberta from 1935 until 1937.
Joseph Harry René Tremblay (September 21, 1899 – November 26, 1990) was a provincial politician from Alberta, Canada.
Leonidas Alcidas Giroux (July 26, 1885 – September 7, 1936) was a provincial politician from Alberta, Canada.
Lethbridge was a provincial electoral district in Alberta, Canada.
The Mayo Clinic is a nonprofit academic medical center based in Rochester, Minnesota focused on integrated clinical practice, education, and research.
Okotoks-High River was a provincial electoral district in Alberta, Canada.
Peter McGregor Campbell (February 9, 1872 – September 19, 1954) was a provincial politician from Alberta, Canada.
The Progressive Conservative Association of Alberta (often referred to colloquially as Progressive Conservative Party of Alberta) was a provincial centre-right party in the Canadian province of Alberta.
Samuel Augustus Gordon Barnes (August 10, 1875 – April 14, 1941) was a teacher, insurance salesman and politician from Alberta, Canada.
Stettler was a provincial electoral district in Alberta, Canada.
Stony Plain originally styled Stonyplain is a provincial electoral district in Alberta, Canada.
Taber was a provincial electoral district in Alberta, Canada.
Walter Morrish (October 19, 1890 – January 30, 1974) was a provincial politician from Alberta, Canada.
William Aberhart (December 30, 1878 – May 23, 1943), also known as Bible Bill for his outspoken Baptist views, was a Canadian politician and the seventh Premier of Alberta (1935 to his death in 1943).
William Neelands Chant (July 13, 1895 – September 25, 1976) was a farmer and political figure in Alberta and British Columbia.
William Edgar Hayes (April 14, 1879 – April 2, 1939) was a provincial level politician from Alberta, Canada.
William Robinson Howson (March 6, 1883 – June 25, 1952) was a politician, judge, debt collector, soldier banker and real estate agent from Alberta, Canada..


whenever i would find myself sitting in between these two i felt as if i was inside some soiled force field. same position, same facial expression, even tails wagging exactly the same – eerie, eerie, eerie. demeter has been really angry at garcia ever since she got sick and now that gar's gone she's been pretty depressed. she's been informed that she's not going anywhere and needs to stay with us for the foreseeable future.


text:
Q: How to fix "Cookie set without httpOnly" security Issue in GWT We have developed a web application using Java and GWT, Now we are fixing the following issues:
Security Issues:

*

*X-Frame-Options:

*X-XSS-Protection:

Cookie:

*HttpOnly and Secure

From the above 3 issues we are able to fix the first 2 issues but unable to fix third issue, because we are accessing cookies created by server at client side which is developed with GWT(javascript). So We are thinking that, it can not be fixed for our application Or can it be ignored because we fixed for "X-Frame-Options" which disallows javascript injection into our website.
Please give me suggestion about our above issue.

A:
HttpOnly and Secure

You can set the secure flag on cookies and you will still be able to access them via JavaScript. Please note that the whole of the application that uses GWT will need to be accessed over https for this to work.
If your application requires that all cookies are read via JavaScript then you cannot set the http only flag. Please note that this is only important for session or authentication cookies - if it is possible to set those to http only and leave your others without the flag then this is the way to go.
Note that X-Frame-Options does not provide any more protection against JavaScript injection into your website than normal. The Same Origin Policy does this as standard. X-Frame-Options simply prevents your site loading into a frameset or IFrame to mitigate clickjacking.

A: The GWT Cookies.setCookie method doesn't support HttpOnly.  You can just create your own setCookie method to set it if you like.  However, you won't be able to read the cookie from JavaScript if you do.
I needed to set the cookie value SameSite to be Lax, so just created the following method:
public static native void setCookie(String name, String value, double expires, boolean secure) /*-{
    var c = name + '=' + value;
    if (expires)
        c += ';expires=' + (new Date(expires)).toGMTString();
    if (secure)
        c += ';secure;SameSite=Lax';
    $doc.cookie = c;
}-*/;

Easy!  :)


WOW! Momo, a Kolkata-based branded momo chain, has raised over Rs 10 crore in its first round of funding from Naukri.com's founder Sanjeev Bikhchandani and Indian Angel Network (IAN).
Investors like Saurabh Srivastava, Ashvin Chadha, Ajai Chowdhry, Kris Gopalakrishnan, Raman Roy, Anand Ladsariya, amongst others also participated in the funding round. The company was valued at $10 million.
Commerce graduates Sagar Daryani and Binod Kumar Homagai founded WOW! Momo in 2008 with an initial investment of Rs 30,000. They have grown the QSR chain to 50 outlets across six in India such as Kolkata, Bangalore, Pune, Chennai, and Kochi.
The company will use the funds to expand its presence with 60 more stores across major cities in India out of which 30 will be based out of Delhi. They will be in high street locations, outlets in malls in areas such as Lajpat Nagar, Satya Niketan, Prashant Vihar, Kirti Nagar, Dwarka and Noida," says Daryani.
Last week, the company opened its new outlet in the tony Hauz Khas area of New Delhi.
Some of their product innovations include Chocolate Momo, MoBurg, Sizzler Momo's, Baked Momo Augratin etc. because of which their business model is being studied as a case study at various Multi National Organizations and B-Schools.
"We closed FY2014-15 at a turnover of Rs 20 crores and have a monthly run rate of 2.7 crores," informs Daryani, CEO of WOW! Momo.


text:
Рата () — село в Рава-Русской городской общине Львовского района Львовской области Украины.

Население по переписи 2001 года составляло 639 человек. Занимает площадь 1,33 км². Почтовый индекс — 80317. Телефонный код — 3252.

История
В 1946 г. Указом ПВС УССР село Рата переименовано в Подгородное.

В 1995 г. селу возвращено историческое название.

Ссылки
 Рата на сайте Верховной рады Украины

Примечания

redpajama_set_name: RedPajamaWikipedia


text:
Tag: Peter Stastny
Paul Stastny Keeping Up With Father's Legacy
In Stats
Golden Knights center Paul Stastny's father Peter Stastny retired from the NHL when he was 38-years-old. Paul is five years away from reaching that achievement. The older Stastny was inducted into the NHL Hall of Fame in 1998 after registering 1,239 points (450 goals, 789 assists) for the Nordiques, Devils and Blues. In his outstanding career, Peter Stastny averaged 1.27 points per game spanning over 15 seasons, which is seventh best in NHL history.
The upcoming 2019-2020 NHL season, will be Stastny's 13th, totaling 874 games played. He now stands 103 contests away from his father's 977 games played. Clearly both have/had the skill, strength and stamina to be effective for that many games. At the age of 33, both Stastny's averaged high minutes and added close to a point a game. The Golden Knights center had his best points per game average in five seasons, adding .80 points per game. He led all Golden Knights centers, even William Karlsson, who averaged .68 points per game.
In the postseason nothing seems to change. Like his father, Stastny plays an important role even in his mid-thirties. In the seven-game series against San Jose, the veteran center averaged more than a point per game scoring two goals and six assists. Coach Gerard Gallant played his "second" line center for twenty minutes a game and used him heavily in crucial points throughout the series. Last season with Winnipeg, Stastny added 15 points (6 goals, 9 assists) over 17 postseason games. He also led the NHL with three game-winning goals in the 2017-18 playoffs. The Stastny's tend to age well.
The 33-year-old is signed with the Golden Knights for at least the next two seasons. Assuming the organization is still highly competitive, the veteran would likely consider finishing his career in Vegas. Stastny is the perfect second line center now, playing along side friend Max Pacioretty and winger Mark Stone. Also, he could be a great depth center down the road. Heck, maybe playing between Pacioretty and Stone will help Stastny get closer to his father's legendary accomplishments.
Chances are, Stastny will never catch up to his old man's 1,239 NHL points, but the Golden Knight can do one thing his Hall of Fame father couldn't do. And that's hoist the Stanley Cup. Playing with Vegas may be the best chance for the entire family. Remember, brother Yan has a job with the Golden Knights organization too.

redpajama_set_name: RedPajamaCommonCrawl


Here's your peek at Amber's "rockin'" new kit releasing Friday 2/22!
A little something for every music fan! And as always you can win it before it is released!
This would be a fun and interesting kit to win! Can't wait to see the whole shebang!
Beautiful kit! Thanks for the chance.
Love the colors, thank you for the chance!
love the colors. Thanks for the chance.
Wow, that is a fun looking kit from what I can see of it. Thanks for the chance to win it.
THANK you - the kit is great!


text:
YOU POLLED REPUBLICANS, NOW POLL AMERICANS
This appeared yesterday:
An exclusive Suffolk University/USA TODAY Poll finds [Donald] Trump's support largely unshaken after his second impeachment trial in the Senate....
By double digits, 46%-27%, those surveyed say they would abandon the GOP and join the Trump party if the former president decided to create one. The rest are undecided....
Half of those polled say the GOP should become "more loyal to Trump," even at the cost of losing support among establishment Republicans. One in five, 19%, say the party should become less loyal to Trump and more aligned with establishment Republicans....
Eight in 10 say they would be less likely to vote for a Republican candidate who supported Trump's impeachment....
And for good measure:
Asked to describe what happened during the assault on the Capitol, 58% of Trump voters call it "mostly an antifa-inspired attack that only involved a few Trump supporters." That's more than double the 28% who call it "a rally of Trump supporters, some of whom attacked the Capitol." Four percent call it "an attempted coup inspired by President Trump."
This is a poll of Trump voters, and it isn't the only post-riot, post-inauguration, post-impeachment polling limited to the right. Last week, as part of a general survey, Morning Consult posed a question to Republican voters exclusively:
According to a Morning Consult/Politico poll conducted at the conclusion of the Senate's weeklong trial, a majority of Republican voters (54 percent) said they would support Trump in a hypothetical 2024 presidential primary election – matching the share who said the same in late November, before his standing dipped in a survey conducted shortly after the deadly Jan. 6 riot at the Capitol.
Yes, Morning Consult has polled GOP voters three times on this question since the election.
On the one hand, there's some value to this. We learned on January 6, and throughout the period between the election and the inauguration, that a thoroughly Trumpified Republican Party is a serious danger to American democracy and puts many people at risk of serious physical harm. We should know whether the backers of one of our two major political parties have thoroughly rejected the notion that the other major party can win an election legitimately, and whether they dismiss concerns about violent behavior by their ideological soul mates.
On the other hand, these polls seem to be a new variant of the media's many safaris into the heart of Trump country, in which reporters discovered every few weeks that, yes, white male retirees in rural diners who voted for Trump still like Trump.
The next midterms will take place 21 months from now; it's way too early to use polling to try to assess what voters will do then, much less two years later in the presidential election. But if we're going to poll, we should poll everybody. We should try to determine whether Trump and his party have alienated the rest of us.
How do voters say they'd vote in a Trump-Biden rematch -- or in a Trump-Kamala Harris matchup? What about Biden or Harris vs. Donald Trump Jr., Josh Hawley, or (if we want to test candidates who aren't Trump purists) Mike Pence or Nikki Haley? What does generic ballot polling look like -- when voters are asked which party they'd back in a vote for Congress, do Republicans do worse? If they do, does the Democratic share of the vote go up, or have alienated GOP voters moved to "undecided" (because they've heard for forty years that Democrats are evil and can't quite make the switch)?
Poll the whole country if you want to poll 2022 and 2024. It would tell us a lot about how all of America feels right now about events since the election, and about what the Republican Party has become. It's possible that swing voters still don't regard the GOP as completely in thrall to Trump, QAnon, and the Oath Keepers, or it's possible that they don't care. If that's the case, we should know. And if they are alienated, we should know that, so we'll stop treating Republican voters as normative Americans.
MINIMIZING BIDEN'S WIN BY CALLING IT "LUCKY"
WINNING, RETROACTIVELY?
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OF COURSE MARJORIE TAYLOR GREENE WANTS TO LEGISLAT...
NO, THESE DEMS DON'T WANT TO RESTRICT THE PRESIDEN...
REPUBLICANS ARE BETTER AT MARCHING IN LOCKSTEP THA...
REPUBLICANS WON'T PERCEIVE A 1/6 COMMISSION AS BAL...
WHO'S AN EVIL ELITIST? LET'S ASK THE FOLKS ON THE ...
WE WON'T GET WHAT WE NEED FROM TRUMP'S FINANCIAL R...
THE ELEVEN WORDS IN TRUMP'S "PERSECUTION" STATEMEN...
BRUNI: LIMBAUGH'S CRITICS ARE THE REAL MENACE
WHAT IF THEY HAD A CIVIL WAR AND NOBODY FOUGHT?
TED CRUZ WILL BE REELECTED IN 2024
FOR ONCE, A REPUBLICAN GETS ALINSKYED
TRIAL BALLOONS SUNK
THE PARTY OF REAGAN WAS THE PARTY OF TRUMP, AND LI...
TRUMP ISN'T EVEN WAITING FOR LIMBAUGH'S BODY TO GE...
THE "LIBERALS" RESPONSIBLE FOR ALL THE WIND TURBIN...
DON'T BLAME AOC -- TEXAS HAS FAILED TO SOLVE THIS ...
REPUBLICANS WOULD STRIP NANCY PELOSI OF HER COMMIT...
THREE NEW POLLS MAKE IT CLEAR THAT REPUBLICANS HAV...
BET ON LARA, NOT ON SARAH
NO, IT WON'T DO
MITCH McCONNELL IS A PARTISAN HACK WHO PLAYS A PIO...
TRUMP THINKS IT'S ALL A GAME
A SIMPLE ANSWER TO A STUPID QUESTION
REPUBLICANS WON'T CONVICT? MUST BE THE DEMOCRATS' ...
REPORT ON FOX AS IF IT'S PART OF THE GOVERNMENT --...
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I GUESS COURAGE AND PRINCIPLES WOULD BE TOO MUCH T...
HOW REPUBLICANS THINK AND HOW DEMOCRATS THINK


When visiting Carmel Valley, you will want to ensure that your stay is as spectacular as the surrounding area. At San Diego Vacation Rentals, we offer a variety of rental properties that will ensconce you in luxury and comfort.
In Carmel Valley, you will find all sorts of wonderful attractions and activities to enjoy. There are three championship golf courses — Ranch Canada Golf Club, Carmel Valley Ranch Golf Course, and Quail Lodge and Golf Club — where you can take in a round or two. You'll also find numerous tennis courts if that's more your style.
Enjoy a visit to Garland Ranch Regional Park. Here you'll find more than 4,000 acres and activities such as mountain trails for hiking, biking, and horseback riding along the willow-lined banks of the Carmel River. You'll also find trails winding their way to the face of the Santa Lucia Mountains to a spot where you can enjoy views the entire length of the Valley.
Just a short 13 miles from Carmel Valley, you'll find Carmel Valley Village here you can enjoy dining, wine tasting, antique shops and art galleries.
Carmel Valley is a great place to explore the arts. There are many galleries where you can find a variety of artistic styles. Some artists have even opened their studios to the public where you can see works in progress. Because art is so prominent in the area, it's quite possible you'll be enjoying a snack or a meal at one of the area's cafes or restaurants, and you'll find yourself tempted to purchase some of the display art!
An activity not to be missed in the Carmel Valley is visiting the vineyards and wineries. You'll find a variety of vineyards that offer tours and tastings. You can even make it a day and have lunch at a vineyard, and then visit the surrounding art galleries and antique stores.


Bring your friends and family for selfies in the park! Over-sized greeting card frames will be on display in Hurkamp Park.
Bring your friends and family for selfies in the park! Over-sized greeting card frames will be on display in Hurkamp Park. Stop by to visit the cards and take a selfie, share with friends, come back and do it again.
It's FREE to visit the cards and take all the photos you'd like. Featuring four card designs: Merry Christmas, Happy Hanukkah, Happy Kwanzaa and Happy Holidays.


text:
Q: Bounded, measurable and supported on a set of finite measure function Suppose f is a bounded and measurable function on R and supported on a set of finite measure. Prove that for every $\epsilon \gt 0$ there exists a simple function $s$ such that $\int |f-s|dx$ $\lt \epsilon$
I have question: Can I let this simple function be supported on a set of finite measure? Then this simple function will be bounded and measurable and supported, then I can use the linearity of integral and the definition of the integral of this kind of functions to prove that.
I am wondering if I am right. I really appreciate your help if you would like to give me another proof.
Thanks

A: You can choose any simple function that satisfies the condition whether it is supported by finite set or not. In fact, simple function is always bounded and measurable without any condition.

A: We assume that $f$ is supported on $E$ which $m(E)=L<\infty.$ So we can consider a function $f$ on E.
Since $f$ is bounded, it must have a and b such that
$a \leq f(x) \leq b$ for all $x\in E$. Let $N > \frac{L(b-a)}{\varepsilon}.$
We define $E_i = \{x \in E : a+i(b-a)/N \leq f(x) < a+(i+1)(b-a)/N\}$.
Choose $x_i\in E_i$ and define
$ s(x) = \sum_{i=0}^{N} f(x_i) \lambda(E_i)$.
Then you can show that
$|f(x)-s(x)|\leq \frac{\varepsilon}{L}.$
And so on.

A: Let $X$ be the support of $f$ and $\mathbb{1}_X$ its characteristic function. Now observe that $f=f\cdot \mathbb{1}_X$ and that $s \cdot \mathbb{1}_X$ approximate $f$.


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Definition : Simulators designed to produce sounds and murmurs mimicking the timing and pitch of actual heart sounds. In addition to the normal heart sounds, the simulators can mimic other sounds such as clicks, snaps, murmurs, and regurgitation. These simulators usually include an anatomic model of the torso or head, with the neck and torso showing the anatomic landmarks. The torso model is also used to detect and recognize the correct anatomic locations of the sounds. Some of these simulators include capabilities for simultaneous electrocardiograph and/or phonocardiograph display, speakers for auditorium listeners, and auscultation units for group listening of a patient's heart sounds. Heart-sound simulators are used for training of healthcare staff in the auscultation of normal and abnormal heart sounds; some simulators may also include breath and/or bowel sounds.
Entry Terms : "Heart Sound Simulators" , "Heart Sound Training Simulators" , "Simulators, Cardiac, Heart Sound" , "Training Aids, Heart Sound"
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Pinnacle Technology Group, Inc. is pleased to have served our customers in the medical training market for over 30 years and our goal is to continue providing the highest quality state-of-the-art products possible. Our Pinnacle simulators use "Real Patient Data" for a more realistic training experience. We pride ourselves on superior customer service and the relationships we build are long term customer oriented to best serve you.


It's time for another challenge at 613 Avenue Create. This is challenge #133 and the theme is Anything Goes w/optional use a Moon and/or Stars.
This week I made a Christmas card with this cute image that is a clear stamp by Some Odd Girl. I've coloured her with Polychromos, to try my new skin tones. And I'm quite happy with it.
Cute CAS Christmas card in lovely trditional colours. Great colouring of the image. Thanks for joining LLC for our Christmas in July challenge.
Aurora this is a beautiful project with wonderful attention to detail and perfect for our 14th 'ANYTHING GOES' challenge. Thanks for sharing your talent with us. Good luck.


Mint Panel has a presence on www.mintpanel.com/net/org/co.uk. Mint Panel is aware of its obligations under the UK Data Protection Act and is taking active and ongoing steps to address its requirements.
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text:
Phnom Penh Post - Sar Kheng warns officials, security forces against complacency
Sar Kheng warns officials, security forces against complacency
Mech Dara | Publication date 26 April 2018 | 16:33 ICT
Interior Minister Sar Kheng poses with new Kratie Governor Va Thorn. Fresh News
Mech Dara
Interior Minister Sar Kheng told provincial security forces in Kratie on Thursday to remain vigilant for any opposition activity in the run-up to July's national elections, while also warning that a popular opposition movement would only come about from the government's failure to cater to people's needs.
"We must join together to keep, protect and strengthen peace, sovereignty and political stability," he said. "That is the main condition for supporting the process of multiparty liberal democracy and socioeconomic development."
Speaking at the inauguration ceremony of new Kratie Governor Va Thorn, Kheng warned that revolution would only be possible if the people are dissatisfied with the government, though he maintained that the Cambodia National Rescue Party, which secured 44 percent of the popular vote in the 2013 elections, was an illegal entity attempting to sow chaos.
The CNRP was forcibly dissolved last November at the government's behest for allegedly fomenting a foreign-backed "colour revolution", though little evidence has ever been presented.
Kheng on Thursday said the decision was right and lawful.
"The competent authorities . . . must pay attention to prevent and take legal action against any activities that attempt to make Cambodian society fall into chaos [and] turmoil," he said.
However, he noted that any successful anti-government movement would be "born from our inactivity or weakness – from a small issue becoming a big issue".
"Therefore we need to check even the smallest problem, from the tip of our hair to the tip of our toes," he said.
Kheng maintained that the Cambodian People's Party has ruled successfully for decades because it has served the will of the people and made no major mistakes.
"There have been some small mistakes, but they are not serious and it is not dangerous for the country," he said, going on to call for reform at all levels of government.
"I am not blaming but we need to study and learn what we have done that may have made them not vote for us," he said.
This is not the first time Kheng has called for government officials to look inward to find the causes of unrest in Cambodia. In 2016, he also warned that government "inactivity" could lead to revolution.
At the time the comments were in stark contrast with Prime Minister Hun Sen's own rhetoric, which has laid the blame for popular discontent at the feet of criminals and foreign powers.
Paul Chambers, a Southeast Asia expert and lecturer at Naresuan University, said the comments reflect a "personal judgment that the Hun Sen government cannot simply take the people for granted".
"If it is Sar Kheng's standpoint, then this could reflect a distancing of opinion between himself and Hun Sen."
Contact author: Mech Dara
Sar Kheng slams wasted local missions
Sar Kheng: Patriots those who stay with the people, not shout abroad
Kheng calls for inquiry into gun smuggling
PM's son-in-law Dy Vichea gets new security portfolio
Sar Kheng says CNRP stole 'national rescue'
Sar Kheng praised for thwarting 'revolution'
The head of the National Police congratulated Interior Minister Sar Kheng on successfully quashing "colour revolution" in an open letter published on the last day
Kheng seeks constitutional ban on individuals harming Cambodia's 'interests'
Kheng calls for security boost at police meeting
Kheng warns advisers
Sar Kheng says official held in Thailand avoided checkpoint, vows arms probe


text:
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Isn't he amazing! He goes and goes, and doesn't want to stop dancing after the end of the song! He's even trying to sing along!
And by the way, Furbies of all colors can dance! They don't have to be teal. I think the white ones are cutest and they sure can dance too.


text:
Home Health & Medical
in Health & Medical
Netflix's Spanish-language crime series Money Heist is coming to an end. But before we say goodbye to the Professor, Tokyo and the rest of the codenamed gang, there's one final season to end their story.
In the first season, a mysterious man only known as the Professor recruits eight people to carry out an ingenious plan to rob the Royal Mint of Spain. During the heist, the group have to deal with hostages, pressure from the police, and of course, conflict within their own ranks.
Throughout the next few seasons, they manage to escape the bank and make off with the money. But when they all splinter off to enjoy their ill-gotten gains, the police begin to capture the various robbers. The Professor brings them all back in for another heist, this time on the Bank of Spain. And of course, nothing goes exactly as planned.
One of the mainstays of the show is Tokyo, a robber who also serves as an unreliable narrator. Both she and her associates experience love, loss and betrayal while trapped inside the banks. Like any heist that's fun to watch, they also have to come up with inventive plans to stay ahead of the police and their hostages.
Money Heist will keep you guessing at every turn. Trust us, you'll want to see how this one ends. Especially if you're a fan of recent Netflix releases like Army of the Dead and the docuseries Heist. The first five episodes of season five dropped on September 3. There's only five episodes left to complete the show once and for all. Here's everything we know about the upcoming fifth and final installment of Money Heist.
What Happened at the End of Money Heist Season 4?
At the end of season 4, the gang was still trapped in the Bank of Spain. Nairobi is dead, and the police are closing in. When the Professor exposes the unlawful treatment robbers Rio and Lisbon, Inspector Sierra is promptly fired. In retaliation, she decides to take matters into her own hands and go after the Professor herself.
Eventually Lisbon is freed and Sierra finds the Professor. The season ends with Sierra holding him at gunpoint. In season 5, we'll see if all the currently living robbers and the Professor can get out alive.
When Will There Be More Episodes of Money Heist?
The first volume of the fifth and final season of Money Heist aired on September 3, 2021. It consists of five episodes and is only the first half of the show's end.
Volume Two of Money Heist will drop on December 3 with five more episodes, making the final season a grand total of 10 episodes. That means both a fall and winter release for the show, and enough Money Heist to make saying goodbye just a little bit easier.
Milan Polk
Milan Polk is an Editorial Assistant for Men's Health who specializes in entertainment and lifestyle reporting, and has worked for New York Magazine's Vulture and Chicago Tribune.
Tags: carona newscovid newsExplosivehealth newsreadyusa healthusa health news
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text:
Piggy is a 2012 British horror crime film. It is written and directed by Kieron Hawkes, produced by Fulwell 73 and DP Film Productions and starring Martin Compston, Paul Anderson, Ed Skrein and Neil Maskell.

Synopsis
In London, Joe (Compston) enters a depression after his brother is murdered on his way home after a night out, and the police think it looks like an open-and-shut case. However, a man called Piggy (Anderson) arrives claiming to be a mate of the brother and he wants revenge, but is Piggy real or a figment of Joe's imagination?

Cast
Martin Compston as Joe
Rachel Dylan as Claire
Roland Manookian as Craig
Neil Maskell as John
Paul Anderson as Piggy
Ed Skrein as Jamie

Production
The film was produced by Danny Potts and Leo Pearlman for Fulwell 73 and DP Film Productions  with Creativity Media, and directed by Kieron Hawkes. Executive Producer's on the project were Gabe Turner, Joe Moore and Patrick Fischer.

Release
The film had a limited UK cinema release on May 4, 2012.

Reception
On the review aggregator website Rotten Tomatoes, Piggy holds an approval rating of 18% based on 11 reviews.

Critical Reception
Mark Kermode on the Kermode and Mayo's Film Review show on BBC Radio 5Live called it "Death Wish for shoegazers" and "strangely disturbing, ultimately unsatisfying". The Guardian felt it lacked subtlety but compared Anderson's swaggering performance to the character of Tyler Durden in Fight Club.

References

External links

2012 films
British horror drama films
2010s English-language films
2012 horror films


text:
Jessie är ett engelskt smeknamn för Jessica. I Skottland är namnet känt sedan lång tid som ett smeknamn för Jean och diminutiv för Janet. Jessie är en alternativ stavning av pojknamnet Jesse.

Kända personer vid namn Jessie
 Jessie Cave, brittisk skådespelare
 Jessie J, brittisk musiker
 Jessie Jacobs, australisk sångare och skådespelare
 Jessie James, amerikansk musiker
 Jessie Flaws, amerikansk-svensk skådespelare
 Jessie Ståhl, svensk politiker
 Jessie Wessel, svensk skådespelare

Kvinnonamn


text:
The House of Barberini are a family of the Italian nobility that rose to prominence in 17th century Rome. Their influence peaked with the election of Cardinal Maffeo Barberini to the papal throne in 1623, as Pope Urban VIII. Their urban palace, the Palazzo Barberini, completed in 1633 by Bernini, today houses Italy's Galleria Nazionale d'Arte Antica (National Gallery of Ancient Art).

Early history

The Barberini family were originally a family of minor nobility from the Tuscan town of Barberino Val d'Elsa, who settled in Florence during the early part of the 11th century.

Carlo Barberini (1488–1566) and his brother Antonio Barberini (1494–1559) were successful Florentine grain, wool and textile merchants. In 1530 Antonio participated in the defense of the Florentine Republic but after the capture of the city by Imperial troops, and the return to power of the Medici, Antonio grew weary of Medici rule and left Florence in 1537 to oversee Barberini business in Rome.

In 1552, Carlo's son Francesco followed his uncle to Rome and business flourished. Francesco became a very rich man and bought a number of high offices within government and the Catholic church. In 1559, his uncle Antonio was murdered by forces loyal to the Medici.

Francesco continued to build his fortune and amass titles until his death in 1600. Ordinarily his estate would have been "fined" by the Camera Apostolica for operating a business while holding church office but his relatives successfully appealed to the head of the organization Francesco had, himself, once directed. The continuation of Barberini business fell to his nephews (the sons of his brother, also Antonio Barberini, who had died in 1571) including Maffeo Barberini.

Maffeo Barberini as Pope Urban VIII

The Barberini acquired great wealth and influence when Cardinal Maffeo Barberini was elected to the papal throne in 1623, taking the name Pope Urban VIII. He elevated a brother Antonio Marcello Barberini (Antonio the Elder) and two nephews, Francesco Barberini and Antonio Barberini, to the cardinalate. He made another brother Duke of Monterotondo, and gave a third nephew, Taddeo Barberini, the principality of Palestrina. Taddeo was also made Gonfalonier of the Church, Prefect of Rome and Commander of Sant'Angelo.

The ecclesiastical, diplomatic and cultural accomplishments of Urban's reign were overshadowed by the nepotism the pope practised. Urban's contemporary, John Bargrave, wrote:

Likewise, the War of Castro, toward the end of Urban's papacy, sullied Urban's reputation and the popularity of those family members who survived him. It is estimated that during the course of Urban's reign, the Barberini amassed 105 million scudi in personal wealth.

When the pope removed the ancient bronze beams from the portico of the Pantheon to procure bronze for the baldachin of St. Peter's Basilica and for the papal cannon foundry, an anonymous critic punningly wrote:

This translates to "What the barbarians did not do, the Barberini did". The pope erected a tablet proudly proclaiming his re-use of these hidden beams for the glory and defense of the church.

Wars of Castro, exile and restoration

The Barberini participated extensively in the First War of Castro. The conflict began when Odoardo Farnese, Duke of Parma and Piacenza, visited Rome and insulted the pope's nephews by suggesting the brothers were too young to manage the Pope's affairs. The war produced no clear victor, and Pope Urban died in 1644, only months after a peace accord was signed.

Despite Urban's appointment of a number of relatives as cardinals, the College of Cardinals elected Pope Innocent X of the Pamphili family. Almost immediately, Innocent X launched an investigation into the conduct of various members of the Barberini family during the wars.

The three nephews who had risen to prominence under their uncle Pope Urban VIII, cardinals Antonio and Francesco and Prince Taddeo were forced into exile and fled to Paris under the protection of Cardinal Mazarin. Antonio and Taddeo left first, by sea, but not before hanging the French coat of arms above the door of the Palazzo Barberini to confirm they were under the protection of France. Francesco joined his brothers soon after.

Taddeo's wife, Anna Colonna also joined her husband and children in Paris but not before making a passionate appeal (in person) to the Pope, urging him not to strip the Barberini of their assets. The Pope agreed and, though he paid some debts out of the Barberini estate, left the Barberini alone.

In Paris they relied on the hospitality of Louis XIV, King of France, until 1653 when most of the family finally returned to Rome. Though Taddeo died in exile in 1647, his brothers eventually reconciled with the papacy through the marriage of Taddeo's younger son Maffeo with Olimpia Giustiniani, a niece of Pope Innocent. Maffeo was given his father's former title, that of Prince of Palestrina.

Taddeo's older son Carlo Barberini was made a cardinal by Pope Innocent X. Taddeo's daughter, Lucrezia Barberini, married Francesco I d'Este, Duke of Modena (who had previously sided with the Farnese during the First War of Castro), further stabilizing relations.

Later history

The 1627 marriage of Taddeo Barberini and Anna Colonna, daughter of Filippo I Colonna began the century-long process which would eventually see the Barberini merge with the Colonna family.

In 1728, the Carbognano branch (Colonna di Sciarra) of the Colonna family added the name Barberini to its family name when Giulio Cesare Colonna di Sciarra married Cornelia Barberini, daughter of Urbano Barberini, the last legitimate male Barberini heir.

Though Urbano's wives bore him no legitimate male heirs, Urbano fathered a son, Maffeo Callisto Barberini in 1688 prior to any one of his three marriages. The will of Urbano Barberini's last wife, Maria Teresa Boncompagni, makes mention of this Maffeo Callisto as the Marquis of Corese. A large portion of the Barberini estate was left for him in her will.

Later her progeny came into conflict with his over claims to the Barberini estate but the quarrel was settled with an agreement signed in Paris in 1811 which divided the estate between the two claimant branches of the family.

The Colonna line became extinct again on the death of Prince Enrico Barberini-Colonna and the name went to his daughter and heiress Maria and her husband Marquis Luigi Sacchetti, who received the title of Prince of Palestrina and permission to use the Barberini name.

On 21 June 2005, Augusto Barberini, the 13th Prince of Palestrina, died in Rome. The family is now represented by Benedetto Francesco Barberini, Prince of Palestrina (born 1961), whose heir is his eldest son.

Patrons of the arts

The Palazzo Barberini, the Barberini library (now a core section of the Vatican's Biblioteca Apostolica), and the many buildings, altars, and other projects spread across Rome (and marked with the heraldic three bees) give evidence of the family's wealth, taste and magnificence in the seventeenth century. The family commissioned many artists, such as Lorenzo Ottoni, to undertake various Barberini-centric projects. The family were also important early patrons of opera, maintaining "star" singers like Marc'Antonio Pasqualini on payroll, and building the private Teatro delle Quattro Fontane.  Many objects from the Barberini art collections are scattered in museums around the world including:

 The Barberini Faun and Barberini Apollo, sold to Ludwig I of Bavaria and now in the Munich Glyptothek
 The Barberini Venus
 The Barberini Hera, also seen in this head;
 The Portland Vase (once known as the Barberini Vase), bought from the family by Sir William Hamilton and now in the British Museum
 The Allegory of Divine Providence and Barberini Power
 The Anglo-Saxon Barberini Gospels, in the Vatican Library, with many other manuscripts from the Barberini collections
 The Barberini Codex, or Libellus de Medicinalibus Indorum Herbis, an Aztec herbal manuscript now once again in Mexico.

A nucleus remains in the hands of the family, as well as in the Galleria Nazionale d'Arte Antica, which occupies part of the Palazzo Barberini in Rome.  The cultural influence of the dynasty was considerable, and provided the subject for a major international conference in December 2004 (and subsequent publication), entitled I Barberini e la Cultura Europea.

Barberini family tree

Family tree of the 16th and 17th century Barberini (hereditary patriarchy of the family is indicated by the colored squares).

See also

 The Allegory of Divine Providence and Barberini Power
 Ferrante Pallavicino – satirical critic of the Barberini.

References

External links
 Piazza Barberini Rome Italy

Families of post-ancient Rome
Papal families
Italian noble families
People from Barberino Val d'Elsa


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Weight Loss Diets
Four-Week and 1,300-Calorie Meal Plans
Andrew Bennett
Andrew Bennett enjoys exploring health and fitness through his personal workouts, as well as researching the latest about the subject. As a natural body builder, Bennett enjoys the ongoing pursuit of health and wellness in all aspects of life. He writes articles, blogs, copy, and even award-winning screenplays.
While not for everyone, a 1,300-calorie meal plan may lead to healthy weight loss over a four-week period of time. Caloric intake varies significantly depending on your individual body weight, so it would be impractical to prescribe 1,300 calories for all dieters. Always consult with your doctor before beginning any new diet.
A woman is slicing vegetables. (Image: Stockbyte/Stockbyte/Getty Images)
A 1,300-calorie meal plan may not be suitable for all dieters because each individual has a special daily caloric demand that depends on their age, metabolic rate and body weight. Cutting calories below your maintenance intake allows for weight loss. However, reducing your calories too far below this figure can actually work against your metabolism, according to "Xtreme Lean" by Jonathan Lawson and Steve Holman. A 1,300-calorie meal plan may be suitable for a small-framed male or a female with a maintenance caloric intake of 1,800 to 2,000 daily calories.
Many different types of meal plans can help you lose weight. Low-carbohydrate diets, for example, call for eating 30 to 50 g of carbohydrates for five days straight. This carb-depletion phase is followed by 24 to 48 hours of carb-loading in the cyclic ketogenic diet. Carb-tapering refers to eating the majority of your carbohydrates in the morning and afternoon, which decreases the likelihood that excess carbs will get stored as fat. A moderate-carbohydrate diet calls for slightly more carbohydrates, which may make up 40 percent of your total calories.
When following a four-week meal plan program, you must increase caloric intake slightly every one or two weeks to prevent your metabolism from slowing down, says "The Abs Diet" by David Zinczenko. For example, having one cheat meal per week, where you eat anything you want actually speeds up metabolic rate. In his book "The Holy Grail Body Transformation Program," Tom Venuto calls this "re-feeding" because it prevents the body from entering dieting plateaus.
You subtract 500 to 750 calories per day from your maintenance figure to create caloric deficit. If you take in five to six small meals and snacks per day, your 1,300 calories breaks down into 260 calories per meal. Alternatively, you could drink 20 g whey protein shakes between meals to speed metabolism your remaining three meals would allot 380 calories each. Shilstone's optimal fat-burning macronutrient ratio recommends 30 percent protein, 30 percent fat and 40 percent carbohydrate. Therefore, each meal would contain approximately 28.5 g protein, 38g carbs and 12.6 g of fat.
Zinczenko recommends taking in 1 g protein per 1 lb. of your body weight each day. For example, a 100-lb. female would try to get at least 20 g lean protein at each of her five daily meals and/or snacks. The remaining calories should come from dietary carbohydrates and fats. Shilstone recommends choosing low-glycemic carbohydrates like oatmeal, sweet potatoes, quinoa and whole-grain pasta and breads. Healthy fats, like olive oil, egg yolks, avocados, nuts and seeds, make excellent choices because they actually help your body burn more fat, according to "The Usual Suspects" by Jordana Brown.
"Xtreme Lean"; Jonathan Lawson and Steve Holman; 2005
"The Abs Diet"; David Zinczenko; 2004
"The Holy Grail Body Transformation Program"; Tom Venuto; 2010
"Combat the Fat"; Jeff Anderson; 2008
"Muscle & Fitness Presents 2010 Edition: The Ultimate Supplement Handbook"; The Usual Suspects; Jordana Brown; January 2010
Macronutrient Ratios in a Diet
1000 Calorie Per Day High Protein Diet
How To Calculate My Recommended Dietary Allowance
1,400 Calorie Diet Menu Plan
Hardcore Bodybuilding Cutting Meal Plan
Caloric Intake for Soccer Players


Here in Northern Kentucky, riding season is temporarily on hold due to winter weather. For those of you who are planning to squeeze a few more motorcycle roads trips in these seasons in more travel-friendly weather in sunny California, we thought it would be helpful to share a list of tips for avoiding a tip over on your next ride. Below, we've posted several tips, courtesy of Ken Condon for MotorcyclistOnline.com. Safe travels!
Learn slow-speed riding techniques: With practice, Condon says, you can learn to maneuver your bike at slow speeds and reduce the risk of tipping over. The key, he says, is to maintain steady drive by keeping the throttle fixed while slipping the clutch and dragging the rear brake to control speed. Also, be sure to look over your shoulder as you lean the bike beneath you. For tighter turns, weight the outside footpeg.
Maintain a stable speed: Condon says that gyroscopic and inertial forces keep your motorcycle stable. Therefore, adding just 1-2 mph will improve stability dramatically.
Square the handlebars when stopping: Condon advises riders to straighten the motorcycle as you smoothly apply the brakes, making sure the bike is completely vertical with the handlebars "square" before finishing the stop.
Keep your eyes up: Condon says that keeping your eyes and vision at eye level will help maintain balance and allow you to spot hazards early.
Favor the rear brake: It's easy to introduce too much front brake force too abruptly, which can cause the bike to stop suddenly before you can straighten it out. Therefore, Condon says, brake cautiously.
Choose your footing: Condon recommends wearing footwear with oil-resistant, tread-like soles to minimize the likelihood of having a foot slide out from under you on slippery substances, such as sand, gravel, or vehicle drippings.
Located just outside Los Angeles, South Bay Sport Bike Rentals services the Southern California area with top of the line motorcycle rentals. The current stable offering at South Bay includes the Triumph Daytona, Yamaha R6, Honda CBR and more that can be found at their available motorcycle rentals page. The friendly staff at South Bay is headed by Jeff Marchesani who granted Rent It Today an interview in 2014 that can be read here.
South Bay Sport Bike Rentals is located in prime motorcycle touring country–sure to give riders a glimpse of the some of the most beautiful scenery in the southwest United States. Local favorite touring locations include Angeles Crest Highway, Ortega Highway, Mt. Palomar and the Malibu Canyons.