Computing osculating orbital elements

Click For Summary

Discussion Overview

This discussion revolves around the calculation of orbital parameters for solar system bodies, specifically focusing on the choice between heliocentric and barycentric coordinates, as well as the reference frame for equinox and ecliptic. Participants explore the implications of these choices on the resulting orbital elements and their discrepancies with established values.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants suggest that position and velocity can be either heliocentric or barycentric, with the choice affecting the resulting orbital elements.
  • It is noted that using barycentric coordinates for Earth may not be sensible due to its position relative to other solar system bodies.
  • There is a discussion about the interpretation of the ascending node values, with one participant mentioning that -11 degrees and 349 degrees represent the same angle.
  • Participants highlight that the calculated Longitude of Ascending Node can vary significantly due to the lack of inclination in Earth's orbit, which is influenced by perturbations from other celestial bodies.
  • One participant emphasizes the importance of consistency in the reference frame used when comparing results with published data, such as that from NASA.
  • Another participant shares their experience of calculating state vectors from Horizons' orbital elements and notes that their results were close, differing only by small decimal values.

Areas of Agreement / Disagreement

Participants generally agree on the importance of the reference frame and coordinate system in orbital calculations, but there are differing views on the implications of using barycentric versus heliocentric coordinates, as well as the interpretation of specific orbital element values.

Contextual Notes

Participants mention that discrepancies in calculated values may arise from differences in the data sets used, such as whether the position and velocity are measured or computed, and the specific reference frame applied (e.g., J2000 vs. mean of date).

Who May Find This Useful

This discussion may be useful for individuals interested in orbital mechanics, astrodynamics, and those working on calculations involving celestial bodies in the solar system.

cptolemy
Messages
45
Reaction score
1
Good afternoon,

I wonder if someone can help me in a small doubt.

I'm trying to calculate the orbital parameters of some solar system bodies. It's quite easy knowing their positions and velocities.

But my question is this: these two components, position and velocity, must they be heliocentric or barycentric?

And as far the equinox and ecliptic of reference, must it be the J2000 or the mean of date?

I'm asking this, because I get different ascending nodes, for instance for Earth, compared to the NASA release values. Actually, their value is for J2000 about -11 degrees, which is strange; it should be a positive number (adding 360).

Does anyone has expertise in this field?

Cheers,

Kepler
 
Astronomy news on Phys.org
Position and velocity can be either heliocentric or barycentric. If you use heliocentric position and velocity, you'll get heliocentric orbital elements.

For computing Earth's orbital elements, it doesn't make much sense to use barycentric since Earth orbits inside the orbit of Jupiter, the Sun's biggest perturber.

-11 and 349 are just 2 ways of saying the same thing. Where is the NASA page that states -11 degrees? Using Horizons, I get 160 degrees.

Regardless, it's not surprising to get vastly different numbers when computing the ascending node of an orbit with no inclination. Since Earth's orbit defines the ecliptic plane, Earth has no inclination. Only the z-component tugs from the Moon and other planets barely give Earth an instantaneous non-zero inclination, but it changes all the time, causing Earth's calculated Longitude of Ascending Node to dance all over the place.

You'll get similar poorly-defined results if you try to compute Earth's argument of perihelion, since it's measured from the poorly-defined LAN.

To a lesser degree, Venus' argument of Perihelion dances all over the place too, since its orbit is very circular. A perfectly-circular orbit has no perihelion.

How do your computed values compare to NASA's values for other orbital elements?
 
cptolemy said:
Good afternoon,
But my question is this: these two components, position and velocity, must they be heliocentric or barycentric?
And as far the equinox and ecliptic of reference, must it be the J2000 or the mean of date?
Depends on what you want out of it. If you start with heliocentric, J2000 pos/vel, you will get heliocentric, J2000 orbital elements. Just be careful in doing your comparisons with someone else's results (even NASA's) - if they started with, for instance, barycentric, J2000 pos/vel, their results will be different. Or, if they started with some other data set - pos/vel as measured by a spacecraft rather than pos/vel computed and published in an almanac - again, different results if you happen to be comparing yours to the almanac elements.

The best thing to do, if you're verifying a set of equations or something, is to find some output data with known input data and put that through your program.
 
  • Like
Likes   Reactions: cptolemy
Hi everyone,

Thanks for trying to help. Oh, and of course, thank you very much for mention the "great Jean Meeus" - one of my idols regarding time fit astronomical alghorythms. I have - I think - all his books. Willman Bell is a great provider of specific astronomy technical books that we do not find elsewhere...

I did some digging - and reversed the problem. Calculated the state vectors of Horizons from their orbital elements. Conclusion: they were diferent from mine... thus the difference.

Horizons calculates the simple vectors choice in barycentric coordinates. As for the orbital elements, it's calculation is made in heliocentric ones, referred to the equinox and equator plane of J2000, TDB scale (or similar - they use Coordinate Time), with true coordinates - no light effect, aberration or whatever. Not astrometric - just true.

I'm getting now very similar results since my state vectors differ only in some decimals (10^-9 aprox.). But the results are quite accurate, I must say :)

So, up until next time.

Cheers,

CPtolemy
 

Similar threads

  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 3 ·
Replies
3
Views
5K
  • · Replies 4 ·
Replies
4
Views
5K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 2 ·
Replies
2
Views
5K
  • · Replies 7 ·
Replies
7
Views
5K
  • · Replies 1 ·
Replies
1
Views
2K
Replies
13
Views
4K
  • · Replies 2 ·
Replies
2
Views
4K
  • · Replies 45 ·
2
Replies
45
Views
83K