<p>In addition to the small z-coordinate discrepancy explained in the previous answer and links, the assertion that the x-coordinate should be 1 AU at JD 2451545, and the y-axis zero, is incorrect. In the question you included the following:</p>

<blockquote>
  <p>X-axis : out along ascending node of instantaneous plane of the
  Earth's orbit and the Earth's mean equator at the reference epoch</p>
</blockquote>

<p>In other words, the x-axis points outward from the Vernal equinox at the J2000.0 epoch along the line of nodes, which is the intersection of the ecliptic and equatorial planes. The Sun is about 2 2/3 months away from the ascending node on Jan 1, so the Earth-Sun radius is not directly on the x-axis.</p>

CC BY-SA 4.0
2019-07-16T05:51:38.657Z
Ok - thank you very much, I didn’t understand properly what it meant. By the way, I couldn’t see on the NASA website where they define the y axis, only x and z. I assume that xyz is a right handed coordinate system... and not xzy?
Bruce Bartlett
CC BY-SA 4.0
2019-07-15T15:55:23.127Z
2019-07-15T15:55:23.127Z
amateurAstro
<p>You made the same fundamental mistake that Anton Gromov made in <a href="https://space.stackexchange.com/questions/18645">his question</a> on the sister <a href="https://space.stackexchange.com">Space Exploration</a> StackExchange network site: You used the solar system barycenter rather than the Sun as the frame origin. Had you used the Sun, the apparent discrepancy would have dropped by almost two orders of magnitude.</p>

<p>A much lesser flaw is that you apparently used midnight rather than noon. The J2000.0 epoch is 12 noon Terrestrial Time on 1 January 2000. This doesn't change things by much, but it is nonetheless important. That half day offset has bitten me more than once.</p>

<p>The z coordinate of the Earth's position would not have dropped to zero had you made the above corrections (Sun-centered rather than solar system barycenter, and 12 noon rather than midnight). It would not have dropped to zero even if you had used the Earth-Moon barycenter rather than the center of the Earth.</p>

<p>One reason it would not have dropped to zero is that the Earth's orbit about the Sun is not an ellipse. The Earth's orbit doesn't even lie on a plane! The key cause of this non-planar motion is that the Moon's orbit about the Earth is inclined by about 5.15° with respect to the ecliptic, making the Earth bob up and down with respect to the ecliptic<sup>1</sup>. Because the Earth's orbit is not truly elliptical or even planar, the ecliptic plane at some epoch is a time-averaged plane centered about the epoch time that makes the Earth's position with respect to the Sun (or the Sun's position with respect to the Earth) average to zero.</p>

<p>A lesser reason is that the J2000.0 mean ecliptic and mean equinox frame was defined over 36 years ago. HORIZONS uses DE431, which was released 6 years ago. JPL's ability to model the solar system improved significantly in the intervening three decades.</p>

<p><br>
<sub><sup>1</sup> Strictly speaking, it makes the Sun appear to bob up and down with respect to the ecliptic. The concept of the ecliptic plane dates back to the ancient Greeks, and it retains a vestige of this definition to this day.</sub></p>

CC BY-SA 4.0
2019-07-14T16:47:01.940Z
2019-07-14T16:47:01.940Z
David Hammen
<p>When I go to the NASA HORIZONS webpage</p>

<p><a href="https://ssd.jpl.nasa.gov/horizons.cgi" rel="noreferrer">https://ssd.jpl.nasa.gov/horizons.cgi</a></p>

<p>and ask for the VECTOR coordinates of the Earth on 1 January 2000, it tells me that Earth has the following coordinates in the J2000 epoch:</p>

<p>X =-1.756637922977122E-01 Y = 9.659912850526895E-01 Z = 2.020629118443605E-04</p>

<p>These are measured in astronomical units. Quoting from the webpage:</p>

<hr>

<p>Reference epoch: J2000.0</p>

<p>XY-plane: plane of the Earth's orbit at the reference epoch</p>

<p>X-axis  : out along ascending node of instantaneous plane of the Earth's             orbit and the Earth's mean equator at the reference epoch</p>

<p>Z-axis  : perpendicular to the xy-plane in the directional (+ or -) sense              of Earth's north pole at the reference epoch.</p>

<hr>

<p>But these figures don't make sense! The z value should be EXACTLY zero, since we are measuring at 1 January 2000. Also the x should be exactly 1, and the y should be zero. </p>

<p>What is going on?</p>

<orbit><nasa><ephemeris>
Why does the Earth have a z-component at the start of the J2000 epoch?
Bruce Bartlett
# Why does the Earth have a z-component at the start of the J2000 epoch?

(Asked by: username_0 on 2019-07-14)

When I go to the NASA HORIZONS webpage

<https://ssd.jpl.nasa.gov/horizons.cgi>

and ask for the VECTOR coordinates of the Earth on 1 January 2000, it tells me that Earth has the following coordinates in the J2000 epoch:

X =-1.756637922977122E-01 Y = 9.659912850526895E-01 Z = 2.020629118443605E-04

These are measured in astronomical units. Quoting from the webpage:

---

Reference epoch: J2000.0

XY-plane: plane of the Earth's orbit at the reference epoch

X-axis : out along ascending node of instantaneous plane of the Earth's orbit and the Earth's mean equator at the reference epoch

Z-axis : perpendicular to the xy-plane in the directional (+ or -) sense of Earth's north pole at the reference epoch.

---

But these figures don't make sense! The z value should be EXACTLY zero, since we are measuring at 1 January 2000. Also the x should be exactly 1, and the y should be zero.

What is going on?

**Tags:** orbit, nasa, ephemeris


---

## 2 answers

### Answer by username_2 on 2019-07-14. Score: 28 | Accepted answer

You made the same fundamental mistake that Anton Gromov made in [his question](https://space.stackexchange.com/questions/18645) on the sister [Space Exploration](https://space.stackexchange.com) StackExchange network site: You used the solar system barycenter rather than the Sun as the frame origin. Had you used the Sun, the apparent discrepancy would have dropped by almost two orders of magnitude.

A much lesser flaw is that you apparently used midnight rather than noon. The J2000.0 epoch is 12 noon Terrestrial Time on 1 January 2000. This doesn't change things by much, but it is nonetheless important. That half day offset has bitten me more than once.

The z coordinate of the Earth's position would not have dropped to zero had you made the above corrections (Sun-centered rather than solar system barycenter, and 12 noon rather than midnight). It would not have dropped to zero even if you had used the Earth-Moon barycenter rather than the center of the Earth.

One reason it would not have dropped to zero is that the Earth's orbit about the Sun is not an ellipse. The Earth's orbit doesn't even lie on a plane! The key cause of this non-planar motion is that the Moon's orbit about the Earth is inclined by about 5.15° with respect to the ecliptic, making the Earth bob up and down with respect to the ecliptic1. Because the Earth's orbit is not truly elliptical or even planar, the ecliptic plane at some epoch is a time-averaged plane centered about the epoch time that makes the Earth's position with respect to the Sun (or the Sun's position with respect to the Earth) average to zero.

A lesser reason is that the J2000.0 mean ecliptic and mean equinox frame was defined over 36 years ago. HORIZONS uses DE431, which was released 6 years ago. JPL's ability to model the solar system improved significantly in the intervening three decades.

1 Strictly speaking, it makes the Sun appear to bob up and down with respect to the ecliptic. The concept of the ecliptic plane dates back to the ancient Greeks, and it retains a vestige of this definition to this day.


---

### Answer by username_1 on 2019-07-15. Score: 2

In addition to the small z-coordinate discrepancy explained in the previous answer and links, the assertion that the x-coordinate should be 1 AU at JD 2451545, and the y-axis zero, is incorrect. In the question you included the following:

> X-axis : out along ascending node of instantaneous plane of the
> Earth's orbit and the Earth's mean equator at the reference epoch

In other words, the x-axis points outward from the Vernal equinox at the J2000.0 epoch along the line of nodes, which is the intersection of the ecliptic and equatorial planes. The Sun is about 2 2/3 months away from the ascending node on Jan 1, so the Earth-Sun radius is not directly on the x-axis.

> **Comments:**
> **username_0**: Ok - thank you very much, I didn’t understand properly what it meant. By the way, I couldn’t see on the NASA website where they define the y axis, only x and z. I assume that xyz is a right handed coordinate system... and not xzy?  

---

