<p>By <strong>latitude</strong> and <strong>longitude</strong> of the sun, I think you mean <strong>latitude</strong> and <strong>longitude</strong> of a point on the earth's surface where the rays of the sun fall perpendicular to the surface. </p>

<p>In astronavigation, this point is called the <strong>Geographical Position</strong> (GP) of the sun and terminology to describe this point is slightly different:-</p>

<p><strong>Latitude</strong> of the GP is called <strong>Declination</strong>, and it is numerically equal to what one might call "Latitude". It is measured in degrees North or South the equator. </p>

<p><strong>Longitude</strong> of the GP is called <strong>Greenwich Hour Angle</strong> (GHA). Just like longitude, GHA is measured East or West of Greenwich Meridian. </p>

<p>Describing the sun's position in this way is called the Equatorial Coordinate System.</p>

<p>The Wikipedia page you have used gives the additional formulae below to convert from Ecliptic Coordinates (the steps you followed) to Equatorial Coordinates. </p>

<p><a href="https://i.sstatic.net/4anh0.png" rel="nofollow noreferrer"><img src="https://i.sstatic.net/4anh0.png" alt="enter image description here"></a></p>

<p>Follow these steps to determine Declination <span class="math-container">$\delta$</span> (Equivalent to Latitude).</p>

<p>To get the sun's GHA, you need to first calculate <span class="math-container">$RA$</span> (Right Ascension) as shown above and then convert this to GHA by these= rules...</p>

<p><span class="math-container">$SHA° = 360 – 15 · RA[h] $</span></p>

<p><span class="math-container">$GHA_{Aries}° = 15 · GST[h] $</span></p>

<p><span class="math-container">$GHA = SHA + GHA_{Aries}$</span></p>

<p>For the second step, you will need <span class="math-container">$GST$</span> (Greenwich Sidereal Time) which is you can calculate if you know UT (UT can be obtained from the time shown by a clock). Use <a href="http://www.astro.umd.edu/~jph/GST_eqn.pdf" rel="nofollow noreferrer">this link to convert directly from UT to GST</a></p>

<p>If you want a simple, concise way to be able to calculate the positions of all manner of celestial bodies, the sun, moon, planets, stars, then I highly recommended the book <em>Astronomical Formulae for Calculators</em> by <em>Jean Meeus</em>. It is the simplest, most comprehensive collection of astronomical formulae you are likely find anywhere on earth.</p>

CC BY-SA 4.0
2020-03-20T19:59:12.947Z
Isn't the longitude the negative of the GHA of the Sun? https://en.wikipedia.org/wiki/Hour_angle says hour angles are negative-to-east, but longitudes are typically negative-to-west, right?
nmr
CC BY-SA 4.0
2017-03-31T23:34:28.973Z
2020-05-13T20:35:56.743Z
2020-05-13T20:35:56.743Z
vu2aeo
<p>If you don't need this precisely, the easy way to figure this out would be the following:</p>

<p>You can assume that at noon UTC on one of the equinoxes, the Sun will be directly over (0N, 0E). The longitude of the sub-Solar point will then progress evenly over the course of a day: 4 hours later it's at 60W, 12 hours later at 180W, 18 hours later 90E, etc.</p>

<p>The latitude of the sub-Solar point will either increase or decrease (depending upon the starting equinox) as a sine curve with a period of year and an amplitude equal to the axial tilt of the Earth (23.43705 degrees).</p>

<p>That will be good to ~5 degrees over the course of the year.</p>

<p>To get a more precise answer, you'd need to calculate the Analemma over the course of the year, and position the sub-Solar point accordingly. Formally, this would mean calculating the <a href="https://en.wikipedia.org/wiki/Equation_of_time" rel="nofollow noreferrer">Equation of Time</a> and transforming the resulting time offset into a position offset for the sub-Solar point. E.g., <a href="https://en.wikipedia.org/wiki/File:EquationofTimeandAnalemma.gif" rel="nofollow noreferrer">what's happening in this image</a>.</p>

<p>I'm not familiar with how to do that, so hopefully someone else can help - or the simple way above works.</p>

CC BY-SA 3.0
2017-03-31T15:17:11.847Z
Thanks for the answer! That indeed is a way to calculate this, and I will use it in case I fail the current route (as this is more or less a rough approximation). I have edited the question, with some code, and the result, however, I'm failing to understand what do I need - ecliptic/equatorial/horizontal coordinates. Given the numbers in the result, what do I need to do to get long/lat?
Amit
CC BY-SA 3.0
2017-03-31T15:54:52.163Z
Amit, once you get the equatorial coordinates, you should be there. Equatorial coords are for objects in the sky, but you can "project" them down onto the surface of the Earth to find the sub-Solar point. That is: alpha = long., delta = lat.
Thomas
CC BY-SA 3.0
2017-03-31T14:54:54.883Z
2017-03-31T14:54:54.883Z
Thomas
<p>I've implemented what <a href="https://astronomy.stackexchange.com/questions/20560/how-to-calculate-the-position-of-the-sun-in-long-lat/20585#20585">Thomas suggested</a> as an approximation. It seems to do its job for a small rendered globe toy in JavaScript.</p>



<pre><code>function getSunEuler(date) {
        const now = date || new Date();

        // The boilerplate: fiddling with dates
        const soy = (new Date(now.getFullYear(), 0, 0)).getTime();
        const eoy = (new Date(now.getFullYear() + 1, 0, 0)).getTime();
        const nows = now.getTime();
        const poy = (nows - soy) / (eoy - soy);

        const secs = now.getUTCMilliseconds() / 1e3
                + now.getUTCSeconds()
                + 60 * (now.getUTCMinutes() + 60 * now.getUTCHours());
        const pod = secs / 86400; // leap secs? nah.

        // The actual magic
        const lat = (-pod + 0.5) * Math.PI * 2;
        const lon = Math.sin((poy - .22) * Math.PI * 2) * .41;

        return new THREE.Euler(0, lat, lon, 'YZX');
}
</code></pre>

<p>The returned Euler angle can be used to transform an X unit vector to find a point on a sphere where <em>0 N 0 E</em> is at <em>(1, 0, 0)</em>.</p>

<p>I got curious how accurate the solution is and fiddled with <a href="https://rhodesmill.org/skyfield/" rel="nofollow noreferrer">Skyfield</a> a bit to get closer to the truth:</p>



<pre><code>from skyfield.api import Topos, load
ts = load.timescale()
planets = load('de421.bsp')
sun = planets['sun']
earth = planets['earth']
t = ts.utc(2019, 6, 21, 12, 0, 0)

# A rather correct answer can probably be obtained from
earth.at(t).observe(sun).apparent().position.au
# but I ended up being too lazy to calculate the angles myself

# This serves as a convenient workaround for manual verification
np = earth + Topos('90 N', '180 W')
np.at(t).observe(sun).apparent().altaz()
</code></pre>

<p>The approximation seems to be indeed accurate within a few degrees, but is in an different coordinate system. I'd love it if someone could provide a clean solution using skyfield.</p>

CC BY-SA 4.0
2019-05-03T23:26:38.543Z
2019-05-03T23:26:38.543Z
Caesar
<p>I have a world map, and I want to know, given a timestamp, where is the sun located right now, in terms of long/lat.</p>

<p>Here is a website that does that:
<a href="https://www.timeanddate.com/worldclock/sunearth.html" rel="nofollow noreferrer">https://www.timeanddate.com/worldclock/sunearth.html</a></p>

<p>But they do not share the calculations.</p>

<p>How can I calculate the sun's position in earth gps terms given a timestamp?</p>

<p><strong>Edit</strong>: some context</p>

<p>I have a plane that is determined by 2 points on earth, and that plain is perpendicular to the earth in those points. I want to know where is the sun relative to that plane, so I can know if the sun is to the right of it, or to the left of it.</p>

<p>Instead of working in 3 dimensions, I decided to work in 2. I already have that plane in 2D (just a line on the map), now I need to know where the sun is</p>

<p><strong>Edit2</strong>: Using the wiki page <a href="https://en.wikipedia.org/wiki/Position_of_the_Sun" rel="nofollow noreferrer">here</a>, this is what I got so far</p>

<p>Note: The interesting part is <code>getCurrentPosition</code></p>

<pre><code>class Sun {
    private julianTime(timestamp: number) {
        // Source: http://stackoverflow.com/questions/466321/convert-unix-timestamp-to-julian
        return timestamp / 86400 + 2440587.5;
    }

    private convertEclipticEquatorial(lambda: number, beta: number, R: number, n) {
        const epsilon = 23.439 - 0.0000004 * n; // Obliquity of the ecliptic
        console.log("epsilon", epsilon);
        const alpha = Math.atan2(Degrees.cos(epsilon) * Degrees.sin(lambda), Degrees.cos(lambda));
        console.log("alpha", alpha);
        const delta = Math.asin(Degrees.sin(epsilon) * Degrees.sin(lambda)); // declination
        console.log("delta", delta);
    }

    getCurrentPosition(timestamp: number) {
        const JD = this.julianTime(timestamp);
        console.log("JD", JD);

        // Source: https://en.wikipedia.org/wiki/Position_of_the_Sun
        const n = JD - 2451545;
        console.log("n", n);
        const L = (280.460 + 0.9856474 * n) % 360;
        console.log("L", L);
        const g = (357.528 + 0.9856003 * n) % 360;
        console.log("g", g);
        const lambda = (L + 1.915 * Degrees.sin(g) + 0.020 * Degrees.sin(2 * g)) % 360;
        console.log("lambda", lambda);
        const R = 1.00014 - 0.01671 * Degrees.cos(g) - 0.00014 * Degrees.cos(2 * g); // Distance
        console.log("R", R);

        this.convertEclipticEquatorial(lambda, 0, R, n);
    }
}

class Degrees {
    static sin(angle: number) {
        return Math.sin(angle / 180 * Math.PI);
    }
    static cos(angle: number) {
        return Math.cos(angle / 180 * Math.PI);
    }
}

console.log(new Sun().getCurrentPosition(new Date().getTime() / 1000));
</code></pre>

<p>Running this now, gives:</p>

<blockquote>
  <p><code>JD</code> 2457844.130512928 (can confirm, this is correct)</p>
  
  <p><code>n</code> 6299.1305129281245 (simple math)</p>
  
  <p><code>L</code> 9.181612328272422 (simple math)</p>
  
  <p><code>g</code> 85.95292328111373 (simple math)</p>
  
  <p><code>lambda</code> 11.09465308568091</p>
  
  <p><code>R</code> 0.9990992788207762</p>
  
  <p><code>epsilon</code> 23.436480347794827 (can confirm, that is roughly correct)</p>
  
  <p><code>alpha</code> 0.17801325468993906</p>
  
  <p><code>delta</code> 0.0766106706512887</p>
</blockquote>

CC BY-SA 3.0
2017-03-29T15:07:33.210Z
What tools do you have access to? How are you calculating this? If you're trying to do this from scratch, you're in for a rough time.
zephyr
CC BY-SA 3.0
2017-03-29T15:16:28.263Z
@zephyr Well, I have internet access, not much more. I love cracking tough problems. Perhaps can you point me in the right direction?
Amit
CC BY-SA 3.0
2017-03-29T15:21:29.017Z
This is a really tough problem though. There are people at NASA whos entire job is to do just stuff like this. There's no single source I could point you to that would help you do this yourself. Basically though, you'll need an ephemeris for a particular time period, the ability to progress that ephemeris forward in time to your specific date, and then lots of math to convert the ephemeris info into what you need. Your best bet might be to look at some code by someone who's already done something like this (e.g., http://www.clearskyinstitute.com/xephem/) and copy what they've done.
zephyr
CC BY-SA 3.0
2017-03-29T15:33:21.393Z
@zephyr That really helped! In their source code, I found references to VSOP87, and in a page mentioning VSOP87 I read about VSOP. apparently, someone already did all of the hard work, here https://en.wikipedia.org/wiki/Position_of_the_Sun
and those equations have 0.01 degrees precision, until 2050, so I am set for the next 30 years.

Thanks for the point in the right direction!
Amit
CC BY-SA 3.0
2017-03-29T15:35:20.497Z
Glad I could help. I didn't know there was a wiki page with the relevant equations so that's good to know. Feel free to answer your own question and accept it if that information is sufficient for you.
zephyr
CC BY-SA 3.0
2017-03-29T15:36:16.850Z
@zephyr I'll answer it once I have some code taking a timestamp and returning the sun's position
Amit
CC BY-SA 3.0
2017-03-29T17:55:01.153Z
There is an Excel spreadsheet authored by Greg Pelletier that might get want you want.
BillDOe
<the-sun><mathematics>
How to calculate the position of the sun in long/lat?
Amit
# How to calculate the position of the sun in long/lat?

(Asked by: username_0 on 2017-03-29)

I have a world map, and I want to know, given a timestamp, where is the sun located right now, in terms of long/lat.
Here is a website that does that:
https://www.timeanddate.com/worldclock/sunearth.html
But they do not share the calculations.
How can I calculate the sun's position in earth gps terms given a timestamp?
Edit: some context
I have a plane that is determined by 2 points on earth, and that plain is perpendicular to the earth in those points. I want to know where is the sun relative to that plane, so I can know if the sun is to the right of it, or to the left of it.
Instead of working in 3 dimensions, I decided to work in 2. I already have that plane in 2D (just a line on the map), now I need to know where the sun is
Edit2: Using the wiki page here, this is what I got so far
Note: The interesting part is getCurrentPosition
class Sun {
    private julianTime(timestamp: number) {
        // Source: http://stackoverflow.com/questions/466321/convert-unix-timestamp-to-julian
        return timestamp / 86400 + 2440587.5;
    }

    private convertEclipticEquatorial(lambda: number, beta: number, R: number, n) {
        const epsilon = 23.439 - 0.0000004 * n; // Obliquity of the ecliptic
        console.log("epsilon", epsilon);
        const alpha = Math.atan2(Degrees.cos(epsilon) * Degrees.sin(lambda), Degrees.cos(lambda));
        console.log("alpha", alpha);
        const delta = Math.asin(Degrees.sin(epsilon) * Degrees.sin(lambda)); // declination
        console.log("delta", delta);
    }

    getCurrentPosition(timestamp: number) {
        const JD = this.julianTime(timestamp);
        console.log("JD", JD);

        // Source: https://en.wikipedia.org/wiki/Position_of_the_Sun
        const n = JD - 2451545;
        console.log("n", n);
        const L = (280.460 + 0.9856474 * n) % 360;
        console.log("L", L);
        const g = (357.528 + 0.9856003 * n) % 360;
        console.log("g", g);
        const lambda = (L + 1.915 * Degrees.sin(g) + 0.020 * Degrees.sin(2 * g)) % 360;
        console.log("lambda", lambda);
        const R = 1.00014 - 0.01671 * Degrees.cos(g) - 0.00014 * Degrees.cos(2 * g); // Distance
        console.log("R", R);

        this.convertEclipticEquatorial(lambda, 0, R, n);
    }
}

class Degrees {
    static sin(angle: number) {
        return Math.sin(angle / 180 * Math.PI);
    }
    static cos(angle: number) {
        return Math.cos(angle / 180 * Math.PI);
    }
}

console.log(new Sun().getCurrentPosition(new Date().getTime() / 1000));

Running this now, gives:

JD 2457844.130512928 (can confirm, this is correct)
n 6299.1305129281245 (simple math)
L 9.181612328272422 (simple math)
g 85.95292328111373 (simple math)
lambda 11.09465308568091
R 0.9990992788207762
epsilon 23.436480347794827 (can confirm, that is roughly correct)
alpha 0.17801325468993906
delta 0.0766106706512887

**Tags:** the-sun, mathematics

> **Comments:**
> **username_1**: What tools do you have access to? How are you calculating this? If you're trying to do this from scratch, you're in for a rough time.  
> **username_0**: @username_1 Well, I have internet access, not much more. I love cracking tough problems. Perhaps can you point me in the right direction?  
> **username_1**: This is a really tough problem though. There are people at NASA whos entire job is to do just stuff like this. There's no single source I could point you to that would help you do this yourself. Basically though, you'll need an ephemeris for a particular time period, the ability to progress that ephemeris forward in time to your specific date, and then lots of math to convert the ephemeris info into what you need. Your best bet might be to look at some code by someone who's already done something like this (e.g., http://www.clearskyinstitute.com/xephem/) and copy what they've done.  
> **username_0**: @username_1 That really helped! In their source code, I found references to VSOP87, and in a page mentioning VSOP87 I read about VSOP. apparently, someone already did all of the hard work, here https://en.wikipedia.org/wiki/Position_of_the_Sun and those equations have 0.01 degrees precision, until 2050, so I am set for the next 30 years.  Thanks for the point in the right direction!  
> **username_1**: Glad I could help. I didn't know there was a wiki page with the relevant equations so that's good to know. Feel free to answer your own question and accept it if that information is sufficient for you.  
> **username_0**: @username_1 I'll answer it once I have some code taking a timestamp and returning the sun's position  
> **username_2**: There is an Excel spreadsheet authored by Greg Pelletier that might get want you want.  

---

## 3 answers

### Answer by username_3 on 2017-03-31. Score: 5

By **latitude** and **longitude** of the sun, I think you mean **latitude** and **longitude** of a point on the earth's surface where the rays of the sun fall perpendicular to the surface.

In astronavigation, this point is called the **Geographical Position** (GP) of the sun and terminology to describe this point is slightly different:-

**Latitude** of the GP is called **Declination**, and it is numerically equal to what one might call "Latitude". It is measured in degrees North or South the equator.

**Longitude** of the GP is called **Greenwich Hour Angle** (GHA). Just like longitude, GHA is measured East or West of Greenwich Meridian.

Describing the sun's position in this way is called the Equatorial Coordinate System.

The Wikipedia page you have used gives the additional formulae below to convert from Ecliptic Coordinates (the steps you followed) to Equatorial Coordinates.

[![enter image description here](https://i.sstatic.net/4anh0.png)](https://i.sstatic.net/4anh0.png)

Follow these steps to determine Declination $\delta$ (Equivalent to Latitude).

To get the sun's GHA, you need to first calculate $RA$ (Right Ascension) as shown above and then convert this to GHA by these= rules...

$SHA° = 360 – 15 · RA[h] $

$GHA\_{Aries}° = 15 · GST[h] $

$GHA = SHA + GHA\_{Aries}$

For the second step, you will need $GST$ (Greenwich Sidereal Time) which is you can calculate if you know UT (UT can be obtained from the time shown by a clock). Use [this link to convert directly from UT to GST](http://www.astro.umd.edu/~jph/GST_eqn.pdf)

If you want a simple, concise way to be able to calculate the positions of all manner of celestial bodies, the sun, moon, planets, stars, then I highly recommended the book *Astronomical Formulae for Calculators* by *Jean Meeus*. It is the simplest, most comprehensive collection of astronomical formulae you are likely find anywhere on earth.

> **Comments:**
> **username_4**: Isn't the longitude the negative of the GHA of the Sun? https://en.wikipedia.org/wiki/Hour_angle says hour angles are negative-to-east, but longitudes are typically negative-to-west, right?  

---

### Answer by username_5 on 2017-03-31. Score: 2

If you don't need this precisely, the easy way to figure this out would be the following:

You can assume that at noon UTC on one of the equinoxes, the Sun will be directly over (0N, 0E). The longitude of the sub-Solar point will then progress evenly over the course of a day: 4 hours later it's at 60W, 12 hours later at 180W, 18 hours later 90E, etc.

The latitude of the sub-Solar point will either increase or decrease (depending upon the starting equinox) as a sine curve with a period of year and an amplitude equal to the axial tilt of the Earth (23.43705 degrees).

That will be good to ~5 degrees over the course of the year.

To get a more precise answer, you'd need to calculate the Analemma over the course of the year, and position the sub-Solar point accordingly. Formally, this would mean calculating the [Equation of Time](https://en.wikipedia.org/wiki/Equation_of_time) and transforming the resulting time offset into a position offset for the sub-Solar point. E.g., [what's happening in this image](https://en.wikipedia.org/wiki/File:EquationofTimeandAnalemma.gif).

I'm not familiar with how to do that, so hopefully someone else can help - or the simple way above works.

> **Comments:**
> **username_0**: Thanks for the answer! That indeed is a way to calculate this, and I will use it in case I fail the current route (as this is more or less a rough approximation). I have edited the question, with some code, and the result, however, I'm failing to understand what do I need - ecliptic/equatorial/horizontal coordinates. Given the numbers in the result, what do I need to do to get long/lat?  
> **username_5**: username_0, once you get the equatorial coordinates, you should be there. Equatorial coords are for objects in the sky, but you can "project" them down onto the surface of the Earth to find the sub-Solar point. That is: alpha = long., delta = lat.  

---

### Answer by username_6 on 2019-05-03. Score: 2

I've implemented what username_5 suggested as an approximation. It seems to do its job for a small rendered globe toy in JavaScript.
function getSunEuler(date) {
        const now = date || new Date();

        // The boilerplate: fiddling with dates
        const soy = (new Date(now.getFullYear(), 0, 0)).getTime();
        const eoy = (new Date(now.getFullYear() + 1, 0, 0)).getTime();
        const nows = now.getTime();
        const poy = (nows - soy) / (eoy - soy);

        const secs = now.getUTCMilliseconds() / 1e3
                + now.getUTCSeconds()
                + 60 * (now.getUTCMinutes() + 60 * now.getUTCHours());
        const pod = secs / 86400; // leap secs? nah.

        // The actual magic
        const lat = (-pod + 0.5) * Math.PI * 2;
        const lon = Math.sin((poy - .22) * Math.PI * 2) * .41;

        return new THREE.Euler(0, lat, lon, 'YZX');
}

The returned Euler angle can be used to transform an X unit vector to find a point on a sphere where 0 N 0 E is at (1, 0, 0).
I got curious how accurate the solution is and fiddled with Skyfield a bit to get closer to the truth:
from skyfield.api import Topos, load
ts = load.timescale()
planets = load('de421.bsp')
sun = planets['sun']
earth = planets['earth']
t = ts.utc(2019, 6, 21, 12, 0, 0)

# A rather correct answer can probably be obtained from
earth.at(t).observe(sun).apparent().position.au
# but I ended up being too lazy to calculate the angles myself

# This serves as a convenient workaround for manual verification
np = earth + Topos('90 N', '180 W')
np.at(t).observe(sun).apparent().altaz()

The approximation seems to be indeed accurate within a few degrees, but is in an different coordinate system. I'd love it if someone could provide a clean solution using skyfield.


---

