<p>This is a bit more complicated than it seems. First off, the definition of a day that matters to us earthlings is the average amount of time from one solar noon to the next (or alternatively, the time it takes for the Sun to appear above the same meridian from day to day); it is called a solar day. The sidereal day, which is the time it takes for some given distant star to appear above the same meridian from day to day, is not the one that really matters to us; this is also the amount of time it takes for the Earth to rotate 360 degrees.</p>

<p>While the Earth is rotating on its axis, it is also travelling along its orbit. In about the amount of time it takes to complete one revolution, it has also travelled about one degree along its orbital path so that in order for the Sun to appear above the same meridian, the Earth has to rotate about 361 degrees.</p>

<p>But then near perihelion (its closest approach to the Sun, which is around January) it's travelling even faster, so it has to rotate more than 361 degrees. Near aphelion it's travelling slower, so the Earth has to rotate less than 361 degrees.</p>

<p>As to your actual question, given the complexity of Earth's orbital variations, I'm not sure it's answerable.</p>

CC BY-SA 4.0
2019-03-14T19:04:49.243Z
“*The true solar day tends to be longer near perihelion when the Sun apparently moves along the ecliptic through a greater angle than usual, taking about 10 seconds longer to do so. Conversely, it is about 10 seconds shorter near aphelion. It is about 20 seconds longer near a solstice when the projection of the Sun's apparent motion along the ecliptic onto the celestial equator causes the Sun to move through a greater angle than usual. Conversely, near an equinox the projection onto the equator is shorter by about 20 seconds*” I’m trying to figure out how the perihelion can affect it that much
Autodidact
CC BY-SA 4.0
2019-03-15T09:52:54.097Z
@Autodidact: At perihelion we're about 3.3% closer to the sun than at aphelion, so by Kepler's second law the earth's linear speed relative to the sun is about 3.3% faster. However, being closer to the sun also means that _for each kilometer we move_, the angle to the sun will change by about 3.3% more. These effects add together, so the apparent speed of the sun among the fixed stars is about 6.6% faster at perihelion. This makes the _difference between the solar and sidereal day_ 6.6% larger which indeed works out to around 15 seconds. (Ignoring the effects of axial tilt).
hmakholm left over Monica
CC BY-SA 4.0
2019-03-15T09:58:30.523Z
(There's still a difference of a few seconds from the source you're quoting, but I'll chalk that up to rounding. Remember that "about 10 seconds" has only one significant digit!)
hmakholm left over Monica
CC BY-SA 4.0
2019-03-14T18:29:19.750Z
2019-03-14T18:29:19.750Z
BillDOe
<blockquote>
  <p>Can it be confirmed that it is exactly 360.0 degrees using official data?</p>
</blockquote>

<p><strong>TL;DR:</strong> No, it can not. Instead it can be confirmed to be 361.0 degrees.</p>

<hr>

<h2>To my knowledge:</h2>

<p>The Earth's rotation period is very close to 23 hours, 56 minutes, 4.1 seconds or 86164.1 sec. That's called a <a href="https://en.wikipedia.org/wiki/Earth" rel="noreferrer">sidereal day</a></p>

<p>A day is defined as 24 hours, or 86400.0 sec.</p>

<p>So in one day it turns </p>

<p><span class="math-container">$$360° \times \frac{86400.0}{86164.1} \approx 360.986°$$</span></p>

<p>Rounded "to one decimal point please" that's 361.0°.</p>

<hr>

<h2>Using "Official data":</h2>

<p>NASA Earth Fact Sheet: <a href="https://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html" rel="noreferrer">https://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html</a></p>

<pre><code>Sidereal rotation period (hrs)   23.9345    
Length of day (hrs)              24.0000
</code></pre>

<p><span class="math-container">$$360° \times \frac{24.0000}{23.9345} \approx 360.985°$$</span></p>

<p>Rounded "to one decimal point please" again, that's still 361.0°.</p>

CC BY-SA 4.0
2019-03-15T02:45:52.413Z
@Jasper you're talking about a [solar day](https://en.wikipedia.org/wiki/Solar_time) not a [sidereal day](https://en.wikipedia.org/wiki/Sidereal_time). The question asks about the rotation of the Earth which has to be considered in an inertial frame, and that's what a sidereal day is. A *day* is exactly 24 hours, or 86400 seconds. Solar days aren't really used in time measurement anymore because of the effects you've mentioned.
uhoh
CC BY-SA 4.0
2019-03-14T22:17:33.817Z
2019-03-14T22:17:33.817Z
uhoh
<p>Another way of getting the exact rotation in degrees per day throughout an entire year is to simply take 360 degrees (one extra rotation per year) and divide that by 365 days in the year. That comes to .9863013698630137 degrees MORE per day than one exact rotation of 360 degrees. So the average rotation throughout a year of how many degrees the earth spins,  (according to the heliocentric model), is 360.9863013698630137‬ degrees of rotation per solar day. That means in one hour; 15.0410958904109589 degrees.  </p>

CC BY-SA 4.0
2019-11-09T05:33:58.020Z
The year is closer to 365.25 days than 365.00 days.
Mike G
CC BY-SA 4.0
2019-11-10T06:53:30.637Z
What Mike G said. Also note that there are quite a few ways to define a year, see [Wikipedia](https://en.wikipedia.org/wiki/Year#Astronomical_years). For this application, you could use the sidereal or anomalistic year, or perhaps one of the tropical years.
PM 2Ring
CC BY-SA 4.0
2019-11-08T22:00:30.700Z
2019-11-08T22:00:30.700Z
Larry Thomas Jones
<p>First, we need to decide which definition of "day" to employ. There are several types of days:</p>

<p><strong>Apparent solar day</strong>: the time between two successive culminations of the Sun (apparent Noon) from an fixed Earth-based observer;<br>
<strong>Mean solar day</strong>: a more uniform, averaged solar day without seasonal variations;<br>
<strong>Stellar/Sidereal day</strong>: the time needed for the Earth to rotate once relative to the stars;<br>
<strong>SI day</strong>: a unit of time containing exactly 86,400 SI seconds defined by caesium atoms.</p>

<p>Since we generally refer to the traditional day/night cycle when we say "day", this means a form of solar time. To get a more averaged value, let's use the mean solar day.</p>

<p>The current formula linking the Earth Rotation Angle (ERA) to the modern approximation of mean solar time, UT1 (basically the Earth's clock following the mean day/night cycle), is by definition :</p>

<p><span class="math-container">$$ERA = 2π(0.7790572732640 + 1.00273781191135448 T_u) \text{ radians}$$</span></p>

<p>Where <span class="math-container">$Tu$</span> is the Julian UT1 Date - 2451545.0</p>

<p>So according to this formula, a (UT1) day is 1.00273781191135448 Earth rotations, which multiplied by 360° is about <strong>360.98561°</strong>. However, the Earth's rotation and revolution are not constant, and are always changing at somewhat unpredictable rates, so the angle is not perfect, but the changes are very slow. So this is more a modern approximation rather than an exact value. Rounded to one decimal place, this gives you <strong>361.0°</strong>, a figure that will likely remain true for at least several millenia. </p>

<p>If you want to know the amount of Earth rotation for every SI day, you're in luck: it is possible to consult reports of the Earth's orientation (rotation and polar motion) thanks to the IERS. Values are tabulated for each 0h UTC every day in the IERS publications, allowing to derive the angle that Earth has rotated every 86,400 SI seconds, allowing to scientifically monitor variations in Earth's rotation compared to a very constant unit of time realized by atomic clocks. Nowadays, the Earth's rotation is measured and reported thanks to radio telescopes and <a href="https://en.wikipedia.org/wiki/Very-long-baseline_interferometry" rel="noreferrer">VLBI</a> observing distant objects in the universe. Official reports of its orientation, the <a href="https://www.iers.org/IERS/EN/Science/EarthRotation/EOP.html" rel="noreferrer">Earth Orientation Parameters</a> are published on the <a href="https://www.iers.org/IERS/EN/DataProducts/EarthOrientationData/eop.html" rel="noreferrer">IERS Website</a>. </p>

<p>As an example, here is a graph showing the amount of Earth rotation every 86,400 seconds constructed with IERS data of the last year:</p>

<p><a href="https://i.sstatic.net/ICTX1.png" rel="noreferrer"><img src="https://i.sstatic.net/ICTX1.png" alt="Earth Rotation"></a>
As we can see, there are several seasonal, periodic and unpredictable variations in Earth's rotation.</p>

CC BY-SA 4.0
2019-03-15T05:46:37.227Z
2019-07-16T01:55:36.623Z
2019-07-16T01:55:36.623Z
FSimardGIS
<p>What is the official amount (in degrees, to one decimal point), of the Earth’s rotation in one single day? Can it be confirmed that it is exactly 360.0 degrees using official data?</p>

CC BY-SA 4.0
2019-03-15T11:23:51.757Z
Official according to what or whom?
jpmc26
<earth><rotation>
What is the official amount, in degrees, of the Earth's rotation in a single day?
Autodidact
# What is the official amount, in degrees, of the Earth's rotation in a single day?

(Asked by: username_0 on 2019-03-14)

What is the official amount (in degrees, to one decimal point), of the Earth’s rotation in one single day? Can it be confirmed that it is exactly 360.0 degrees using official data?

**Tags:** earth, rotation
> **Comments:**
> **username_1**: Official according to what or whom?  

---

## 4 answers

### Answer by username_8 on 2019-03-15. Score: 34 | Accepted answer

First, we need to decide which definition of "day" to employ. There are several types of days:

**Apparent solar day**: the time between two successive culminations of the Sun (apparent Noon) from an fixed Earth-based observer;  
**Mean solar day**: a more uniform, averaged solar day without seasonal variations;  
**Stellar/Sidereal day**: the time needed for the Earth to rotate once relative to the stars;  
**SI day**: a unit of time containing exactly 86,400 SI seconds defined by caesium atoms.

Since we generally refer to the traditional day/night cycle when we say "day", this means a form of solar time. To get a more averaged value, let's use the mean solar day.

The current formula linking the Earth Rotation Angle (ERA) to the modern approximation of mean solar time, UT1 (basically the Earth's clock following the mean day/night cycle), is by definition :

$$ERA = 2π(0.7790572732640 + 1.00273781191135448 T\_u) \text{ radians}$$

Where $Tu$ is the Julian UT1 Date - 2451545.0

So according to this formula, a (UT1) day is 1.00273781191135448 Earth rotations, which multiplied by 360° is about **360.98561°**. However, the Earth's rotation and revolution are not constant, and are always changing at somewhat unpredictable rates, so the angle is not perfect, but the changes are very slow. So this is more a modern approximation rather than an exact value. Rounded to one decimal place, this gives you **361.0°**, a figure that will likely remain true for at least several millenia.

If you want to know the amount of Earth rotation for every SI day, you're in luck: it is possible to consult reports of the Earth's orientation (rotation and polar motion) thanks to the IERS. Values are tabulated for each 0h UTC every day in the IERS publications, allowing to derive the angle that Earth has rotated every 86,400 SI seconds, allowing to scientifically monitor variations in Earth's rotation compared to a very constant unit of time realized by atomic clocks. Nowadays, the Earth's rotation is measured and reported thanks to radio telescopes and [VLBI](https://en.wikipedia.org/wiki/Very-long-baseline_interferometry) observing distant objects in the universe. Official reports of its orientation, the [Earth Orientation Parameters](https://www.iers.org/IERS/EN/Science/EarthRotation/EOP.html) are published on the [IERS Website](https://www.iers.org/IERS/EN/DataProducts/EarthOrientationData/eop.html).

As an example, here is a graph showing the amount of Earth rotation every 86,400 seconds constructed with IERS data of the last year:

[![Earth Rotation](https://i.sstatic.net/ICTX1.png)](https://i.sstatic.net/ICTX1.png)
As we can see, there are several seasonal, periodic and unpredictable variations in Earth's rotation.


---

### Answer by username_2 on 2019-03-14. Score: 22

This is a bit more complicated than it seems. First off, the definition of a day that matters to us earthlings is the average amount of time from one solar noon to the next (or alternatively, the time it takes for the Sun to appear above the same meridian from day to day); it is called a solar day. The sidereal day, which is the time it takes for some given distant star to appear above the same meridian from day to day, is not the one that really matters to us; this is also the amount of time it takes for the Earth to rotate 360 degrees.

While the Earth is rotating on its axis, it is also travelling along its orbit. In about the amount of time it takes to complete one revolution, it has also travelled about one degree along its orbital path so that in order for the Sun to appear above the same meridian, the Earth has to rotate about 361 degrees.

But then near perihelion (its closest approach to the Sun, which is around January) it's travelling even faster, so it has to rotate more than 361 degrees. Near aphelion it's travelling slower, so the Earth has to rotate less than 361 degrees.

As to your actual question, given the complexity of Earth's orbital variations, I'm not sure it's answerable.

> **Comments:**
> **username_0**: “*The true solar day tends to be longer near perihelion when the Sun apparently moves along the ecliptic through a greater angle than usual, taking about 10 seconds longer to do so. Conversely, it is about 10 seconds shorter near aphelion. It is about 20 seconds longer near a solstice when the projection of the Sun's apparent motion along the ecliptic onto the celestial equator causes the Sun to move through a greater angle than usual. Conversely, near an equinox the projection onto the equator is shorter by about 20 seconds*” I’m trying to figure out how the perihelion can affect it that much  
> **username_3**: @Autodidact: At perihelion we're about 3.3% closer to the sun than at aphelion, so by Kepler's second law the earth's linear speed relative to the sun is about 3.3% faster. However, being closer to the sun also means that _for each kilometer we move_, the angle to the sun will change by about 3.3% more. These effects add together, so the apparent speed of the sun among the fixed stars is about 6.6% faster at perihelion. This makes the _difference between the solar and sidereal day_ 6.6% larger which indeed works out to around 15 seconds. (Ignoring the effects of axial tilt).  
> **username_3**: (There's still a difference of a few seconds from the source you're quoting, but I'll chalk that up to rounding. Remember that "about 10 seconds" has only one significant digit!)  

---

### Answer by username_4 on 2019-03-14. Score: 15

Can it be confirmed that it is exactly 360.0 degrees using official data?

TL;DR: No, it can not. Instead it can be confirmed to be 361.0 degrees.

To my knowledge:
The Earth's rotation period is very close to 23 hours, 56 minutes, 4.1 seconds or 86164.1 sec. That's called a sidereal day
A day is defined as 24 hours, or 86400.0 sec.
So in one day it turns 
$$360° \times \frac{86400.0}{86164.1} \approx 360.986°$$
Rounded "to one decimal point please" that's 361.0°.

Using "Official data":
NASA Earth Fact Sheet: https://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html
Sidereal rotation period (hrs)   23.9345    
Length of day (hrs)              24.0000

$$360° \times \frac{24.0000}{23.9345} \approx 360.985°$$
Rounded "to one decimal point please" again, that's still 361.0°.

> **Comments:**
> **username_4**: @Jasper you're talking about a [solar day](https://en.wikipedia.org/wiki/Solar_time) not a [sidereal day](https://en.wikipedia.org/wiki/Sidereal_time). The question asks about the rotation of the Earth which has to be considered in an inertial frame, and that's what a sidereal day is. A *day* is exactly 24 hours, or 86400 seconds. Solar days aren't really used in time measurement anymore because of the effects you've mentioned.  

---

### Answer by username_5 on 2019-11-08. Score: 2

Another way of getting the exact rotation in degrees per day throughout an entire year is to simply take 360 degrees (one extra rotation per year) and divide that by 365 days in the year. That comes to .9863013698630137 degrees MORE per day than one exact rotation of 360 degrees. So the average rotation throughout a year of how many degrees the earth spins, (according to the heliocentric model), is 360.9863013698630137‬ degrees of rotation per solar day. That means in one hour; 15.0410958904109589 degrees.

> **Comments:**
> **username_6**: The year is closer to 365.25 days than 365.00 days.  
> **username_7**: What Mike G said. Also note that there are quite a few ways to define a year, see [Wikipedia](https://en.wikipedia.org/wiki/Year#Astronomical_years). For this application, you could use the sidereal or anomalistic year, or perhaps one of the tropical years.  

---

