<blockquote>
<p>Why don't we see a change in temperature when the barycenter changes? </p>
</blockquote>
<p>The motion of the Sun relative to the Solar System barycentre (SSB) doesn't have much of an effect on the Earth's orbit. As the Sun spirals around the SSB it (mostly) drags the planets, moons, asteroids, etc, with it. It's probably best to treat the Sun's location as fixed, with the SSB spiraling around it, especially when analysing the orbits of the smaller bodies in the Solar System. The Sun's motion relative to the SSB is only significant for the giant planets, but even with Jupiter the effect is small because the solar mass is ~1000 times Jupiter's mass.</p>
<p>I have some info and diagrams of the motion of the SSB <a href="https://astronomy.stackexchange.com/a/28036/16685">here</a> and
<a href="https://astronomy.stackexchange.com/a/44903/16685">here</a>.</p>
<p>However, the seasonal variation in the Earth's climate is <em>not</em> primarily due to the change in the distance from the Earth to the Sun. It's mainly due to the change in the angle of the sunlight.</p>
<p>Earth's mean orbital radius is ~149.6 million km, but it varies between ~147.1 and ~152.1 million km, due to the eccentricity of the elliptical orbit (see below). The change in distance due to the axial tilt is relatively small, eg, it's under 3300 km at 40° latitude.</p>
<p>However, the change in the angle of the Sun at noon has a significant impact. As the Earth revolves around the Sun, the axial tilt (~23.44°) causes the Sun's declination on the celestial sphere to vary between -23.44° to +23.44°. This changes the angle of the sunlight at noon. It also affects the times of sunrise and sunset.</p>
<p>From Wikipedia <a href="https://en.wikipedia.org/wiki/Effect_of_Sun_angle_on_climate" rel="nofollow noreferrer">Effect of Sun angle on climate</a></p>
<blockquote>
<p>Seasonal change in the angle of sunlight, caused by the tilt of Earth's axis, is the basic mechanism that results in warmer weather in summer than in winter. Change in day length is another factor.</p>
</blockquote>
<p><a href="https://i.sstatic.net/RRxvV.png" rel="nofollow noreferrer"><img src="https://i.sstatic.net/RRxvV.png" alt="Sun angle projection diagram" /></a></p>
<blockquote>
<p>One sunbeam one mile wide shines on the ground at a 90° angle, and another at a 30° angle. The one at a shallower angle covers twice as much area with the same amount of light energy.</p>
</blockquote>
<p>So when the horizontal angle is 30° (vertical angle = 60°) each unit of area gets half as much energy as when the horizontal angle is 90° (vertical angle = 0°). In general, the intensity is proportional to the sine of the horizontal angle, which equals the cosine of the vertical angle.</p>
<p>This projection effect is also why the Earth is (generally) hottest at the equator and cooler at higher latitudes.</p>
<hr />
<p>You can test the projection effect with a flashlight and a white wall or sheet of paper, but it can be hard to see, especially with a strong light source. That's because it's hard-wired into our visual processing system, so our brains automatically compensate for it, and interpret such brightness changes as angle data. That is, when we see two planes of the same material at slightly different angles, our brains see them as &quot;really&quot; having the same brightness.</p>
<hr />
<p>That Wikipedia quote mentioned that &quot;change in day length is another factor&quot;. I have some info and graphs about that <a href="https://astronomy.stackexchange.com/a/39685/16685">here</a>.</p>
<hr />
<p>The distance from the Earth to the Sun <em>does</em> have an effect on the climate, but it's fairly minor. Currently, the Earth is closest to the Sun (perihelion) in early January, around 10 days after the December solstice, during the  northern hemisphere winter and southern hemisphere summer. That makes the southern summer a bit hotter than the northern summer. It also makes the southern summer a bit shorter, because the orbital speed is fastest near the perihelion. However, the climate in the southern hemisphere is strongly affected by the strong <a href="https://en.wikipedia.org/wiki/Antarctic_Circumpolar_Current" rel="nofollow noreferrer">circumpolar ocean current around Antarctica</a>, which keeps the southern oceans cold all year round. In the southern hemisphere, not many people live at higher latitudes than 40° because it's just too cold, but that latitude in the northern hemisphere is quite heavily populated.</p>
<p>I have some info about the perihelion <a href="https://astronomy.stackexchange.com/a/49605/16685">here</a> and <a href="https://astronomy.stackexchange.com/a/49546/16685">here</a>.</p>
<p>For what it's worth, here's a graph of the distance from the Earth to Sun and to the SSB, for 2022, with a 7 day timestep between the data points.</p>
<p><a href="https://i.sstatic.net/tDLqW.png" rel="nofollow noreferrer"><img src="https://i.sstatic.net/tDLqW.png" alt="Distance from Earth to Sun &amp; SSB, 2022" /></a>
Plotting script from <a href="https://astronomy.stackexchange.com/a/49823/16685">https://astronomy.stackexchange.com/a/49823/16685</a></p>
<p>Here's a plot spanning 1700 to 2200 (the same timespan as my Sun-SSB plot in the answer linked above), also with a 7 day timestep.</p>
<p><a href="https://i.sstatic.net/blL2O.jpg" rel="nofollow noreferrer"><img src="https://i.sstatic.net/blL2O.jpg" alt="Earth to Sun &amp; SSB, 1700 to 2200" /></a></p>

CC BY-SA 4.0
2023-02-12T15:15:17.067Z
For outer solar system objects (objects well beyond Pluto's orbit) it is better to treat such objects as orbiting the solar system barycenter than orbiting the Sun. But for the eight planets, and this is especially true for the four terrestrial planets, it is far better to treat such objects as orbiting the Sun, with the other planets acting as minor perturbing elements.
David Hammen
CC BY-SA 4.0
2023-02-12T15:32:03.580Z
@DavidHammen Good point. https://ssd.jpl.nasa.gov/horizons/news.html says "November 01, 2018: -- The mass-parameter used to compute solar-system barycentric orbital elements (the system GM given in the output header) includes the main-belt mass but does NOT include the Kuiper Belt mass".
PM 2Ring
CC BY-SA 4.0
2023-02-12T15:32:11.633Z
And [Park et al 2021](https://iopscience.iop.org/article/10.3847/1538-3881/abd414) says that DE440 uses "30 KBOs, and a KBO ring representing the main Kuiper belt. [...] The circular KBO ring was modeled as 36 point masses with equal mass located in the ecliptic plane with a semimajor axis of 44 au, with the ring mass estimated".
PM 2Ring
CC BY-SA 4.0
2023-02-12T16:31:42.847Z
It would have been better to plot distances over a much longer span of time, tens to hundreds of years, or even longer.  The Earth-Sun distance would exhibit an almost sinusoidal behavior while the Earth-SSB distance would have lots of beats.
David Hammen
CC BY-SA 4.0
2023-02-12T17:07:06.030Z
@DavidHammen Done. But it looks a bit grungy: the Imgur uploader decided that it's too big and converted it to a JPEG. :(
PM 2Ring
CC BY-SA 4.0
2023-02-12T17:54:20.813Z
But you can see the pattern. The Earth-Sun distance is a nice simple sinusoid with a period of one year. The Earth-SSB distance has beats. Also, clicking on the image shows more detail.
David Hammen
CC BY-SA 4.0
2023-02-12T15:05:51.880Z
2023-02-13T15:54:20.427Z
2023-02-13T15:54:20.427Z
PM 2Ring
<p>I do not have the numbers but I guess the solar system barycenter should move much more than the Earth radius, and if that is correct then it should not be affecting the Earth's temperature.</p>
<p>I mean, even a small change in the proximity to the Sun originated by the axial tilt is causing a big difference in temperatures (summer and winter).</p>
<p>Why don't we see a change in temperature when the barycenter changes? Does it mean that the distance between the Earth and Sun also changes?</p>

CC BY-SA 4.0
2023-02-12T10:05:30.060Z
Does this answer your question? [Is Jupiter warming the Earth? (Earth, Sun Jupiter system)](https://astronomy.stackexchange.com/questions/46708/is-jupiter-warming-the-earth-earth-sun-jupiter-system)
David Hammen
CC BY-SA 4.0
2023-02-12T10:07:18.820Z
You are the person who asked that highly related question. You still seem to be of the impression that the solar system barycenter is a gravitational attractor. It is not. The advantage of a SSB-centered frame is that that frame is the frame in which the equations of motion used in a numerical propagation of the solar system as a whole take on their simplest form. It is highly erroneous to think of individual planets, particularly the four terrestrial planets, as orbiting the solar system barycenter. They orbit the Sun, with the other planets acting as perturbations.
David Hammen
<the-sun><solar-system><earth><temperature><weather>
Is the solar system barycenter affecting the Earth weather?
Enrique
# Is the solar system barycenter affecting the Earth weather?

(Asked by: username_0 on 2023-02-11)

I do not have the numbers but I guess the solar system barycenter should move much more than the Earth radius, and if that is correct then it should not be affecting the Earth's temperature.

I mean, even a small change in the proximity to the Sun originated by the axial tilt is causing a big difference in temperatures (summer and winter).

Why don't we see a change in temperature when the barycenter changes? Does it mean that the distance between the Earth and Sun also changes?

**Tags:** the-sun, solar-system, earth, temperature, weather
> **Comments:**
> **username_1**: Does this answer your question? [Is Jupiter warming the Earth? (Earth, Sun Jupiter system)](https://astronomy.stackexchange.com/questions/46708/is-jupiter-warming-the-earth-earth-sun-jupiter-system)  
> **username_1**: You are the person who asked that highly related question. You still seem to be of the impression that the solar system barycenter is a gravitational attractor. It is not. The advantage of a SSB-centered frame is that that frame is the frame in which the equations of motion used in a numerical propagation of the solar system as a whole take on their simplest form. It is highly erroneous to think of individual planets, particularly the four terrestrial planets, as orbiting the solar system barycenter. They orbit the Sun, with the other planets acting as perturbations.  

---

## 1 answers

### Answer by username_2 on 2023-02-12. Score: 6 | Accepted answer

> Why don't we see a change in temperature when the barycenter changes?

The motion of the Sun relative to the Solar System barycentre (SSB) doesn't have much of an effect on the Earth's orbit. As the Sun spirals around the SSB it (mostly) drags the planets, moons, asteroids, etc, with it. It's probably best to treat the Sun's location as fixed, with the SSB spiraling around it, especially when analysing the orbits of the smaller bodies in the Solar System. The Sun's motion relative to the SSB is only significant for the giant planets, but even with Jupiter the effect is small because the solar mass is ~1000 times Jupiter's mass.

I have some info and diagrams of the motion of the SSB [here](https://astronomy.stackexchange.com/a/28036/16685) and
[here](https://astronomy.stackexchange.com/a/44903/16685).

However, the seasonal variation in the Earth's climate is *not* primarily due to the change in the distance from the Earth to the Sun. It's mainly due to the change in the angle of the sunlight.

Earth's mean orbital radius is ~149.6 million km, but it varies between ~147.1 and ~152.1 million km, due to the eccentricity of the elliptical orbit (see below). The change in distance due to the axial tilt is relatively small, eg, it's under 3300 km at 40° latitude.

However, the change in the angle of the Sun at noon has a significant impact. As the Earth revolves around the Sun, the axial tilt (~23.44°) causes the Sun's declination on the celestial sphere to vary between -23.44° to +23.44°. This changes the angle of the sunlight at noon. It also affects the times of sunrise and sunset.

From Wikipedia [Effect of Sun angle on climate](https://en.wikipedia.org/wiki/Effect_of_Sun_angle_on_climate)

> Seasonal change in the angle of sunlight, caused by the tilt of Earth's axis, is the basic mechanism that results in warmer weather in summer than in winter. Change in day length is another factor.

[![Sun angle projection diagram](https://i.sstatic.net/RRxvV.png)](https://i.sstatic.net/RRxvV.png)

> One sunbeam one mile wide shines on the ground at a 90° angle, and another at a 30° angle. The one at a shallower angle covers twice as much area with the same amount of light energy.

So when the horizontal angle is 30° (vertical angle = 60°) each unit of area gets half as much energy as when the horizontal angle is 90° (vertical angle = 0°). In general, the intensity is proportional to the sine of the horizontal angle, which equals the cosine of the vertical angle.

This projection effect is also why the Earth is (generally) hottest at the equator and cooler at higher latitudes.

---

You can test the projection effect with a flashlight and a white wall or sheet of paper, but it can be hard to see, especially with a strong light source. That's because it's hard-wired into our visual processing system, so our brains automatically compensate for it, and interpret such brightness changes as angle data. That is, when we see two planes of the same material at slightly different angles, our brains see them as "really" having the same brightness.

---

That Wikipedia quote mentioned that "change in day length is another factor". I have some info and graphs about that [here](https://astronomy.stackexchange.com/a/39685/16685).

---

The distance from the Earth to the Sun *does* have an effect on the climate, but it's fairly minor. Currently, the Earth is closest to the Sun (perihelion) in early January, around 10 days after the December solstice, during the northern hemisphere winter and southern hemisphere summer. That makes the southern summer a bit hotter than the northern summer. It also makes the southern summer a bit shorter, because the orbital speed is fastest near the perihelion. However, the climate in the southern hemisphere is strongly affected by the strong [circumpolar ocean current around Antarctica](https://en.wikipedia.org/wiki/Antarctic_Circumpolar_Current), which keeps the southern oceans cold all year round. In the southern hemisphere, not many people live at higher latitudes than 40° because it's just too cold, but that latitude in the northern hemisphere is quite heavily populated.

I have some info about the perihelion [here](https://astronomy.stackexchange.com/a/49605/16685) and [here](https://astronomy.stackexchange.com/a/49546/16685).

For what it's worth, here's a graph of the distance from the Earth to Sun and to the SSB, for 2022, with a 7 day timestep between the data points.

[![Distance from Earth to Sun & SSB, 2022](https://i.sstatic.net/tDLqW.png)](https://i.sstatic.net/tDLqW.png)
Plotting script from <https://astronomy.stackexchange.com/a/49823/16685>

Here's a plot spanning 1700 to 2200 (the same timespan as my Sun-SSB plot in the answer linked above), also with a 7 day timestep.

[![Earth to Sun & SSB, 1700 to 2200](https://i.sstatic.net/blL2O.jpg)](https://i.sstatic.net/blL2O.jpg)

> **Comments:**
> **username_1**: For outer solar system objects (objects well beyond Pluto's orbit) it is better to treat such objects as orbiting the solar system barycenter than orbiting the Sun. But for the eight planets, and this is especially true for the four terrestrial planets, it is far better to treat such objects as orbiting the Sun, with the other planets acting as minor perturbing elements.  
> **username_2**: @DavidHammen Good point. https://ssd.jpl.nasa.gov/horizons/news.html says "November 01, 2018: -- The mass-parameter used to compute solar-system barycentric orbital elements (the system GM given in the output header) includes the main-belt mass but does NOT include the Kuiper Belt mass".  
> **username_2**: And [Park et al 2021](https://iopscience.iop.org/article/10.3847/1538-3881/abd414) says that DE440 uses "30 KBOs, and a KBO ring representing the main Kuiper belt. [...] The circular KBO ring was modeled as 36 point masses with equal mass located in the ecliptic plane with a semimajor axis of 44 au, with the ring mass estimated".  
> **username_1**: It would have been better to plot distances over a much longer span of time, tens to hundreds of years, or even longer.  The Earth-Sun distance would exhibit an almost sinusoidal behavior while the Earth-SSB distance would have lots of beats.  
> **username_2**: @DavidHammen Done. But it looks a bit grungy: the Imgur uploader decided that it's too big and converted it to a JPEG. :(  
> **username_1**: But you can see the pattern. The Earth-Sun distance is a nice simple sinusoid with a period of one year. The Earth-SSB distance has beats. Also, clicking on the image shows more detail.  

---

