Astrometry and Elliptical orbits

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    Orbits
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Discussion Overview

The discussion revolves around the methods for determining the orbits of celestial objects, specifically focusing on astrometry and the challenges posed by elliptical orbits as opposed to circular ones. Participants explore the application of measurements such as distance and angular velocity in calculating orbits, particularly in the context of observational astronomy.

Discussion Character

  • Exploratory
  • Technical explanation
  • Homework-related

Main Points Raised

  • One participant notes that parallax can be used to measure distance to an object orbiting the sun, while angular velocity can be determined by observing positional changes over time.
  • Another participant emphasizes that orbits should be determined based on conic sections rather than circular assumptions, suggesting this approach encompasses all orbital shapes.
  • A participant expresses uncertainty about how to apply measurements of distance and angular velocity to the equations governing elliptical orbits, indicating a need for clarification on the practical application of these concepts.
  • One participant admits a lack of knowledge regarding the calculation of orbits from angular position measurements but references a historical method developed by CFG as potentially valid.
  • A recommendation is made for a textbook that covers orbital determination, highlighting the distinction between practical observational techniques and the theoretical foundations needed for calculations.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the methods for calculating orbits from measurements, and there are varying levels of understanding and expertise regarding the application of these methods.

Contextual Notes

There is an acknowledgment of the complexity involved in deriving orbits from observational data, with some participants indicating a need for further resources and clarification on the mathematical processes involved.

Mu naught
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You can measure the distance to an object orbiting the sun using parallax, and you can determine its angular velocity by measuring its change in position over several hours or days.

From this you can calculate its orbit... if it were circular. However, comets and asteroids follow elliptical orbits, not circular ones. How do you determine the true orbit of an object and its eccentricity?
 
Astronomy news on Phys.org
http://www.schillerinstitute.org/fid_97-01/982_Gauss_Ceres.html

EDIT:
Just read a bit into the paper. Sorry, seems to be crap written by a philosopher. It's 85 pages, though, so maybe there's something worth reading in the rest of the paper.
However, what I wanted to say: You determine orbits not on the assumption of circles, but of conic sections. That covers everything.
 
Last edited:
Ich said:
http://www.schillerinstitute.org/fid_97-01/982_Gauss_Ceres.html

EDIT:
Just read a bit into the paper. Sorry, seems to be crap written by a philosopher. It's 85 pages, though, so maybe there's something worth reading in the rest of the paper.
However, what I wanted to say: You determine orbits not on the assumption of circles, but of conic sections. That covers everything.

thanks i don't have time to look at it now but i will tomorrow. I understand that an ellipse is a conic section, but what I don't really understand is how to apply the measurements you can make - distance and average angular velocity over some interval of time - to the equation for an ellipse.

I should mention the reason I ask is because I'm taking a course in observation astronomy and I'd like to calculate the orbit of comet Hartley for my research project.
 
Actually, what you measure is angular position at different times, and nothing else. I hereby frankly admit that I don't know how to calculate orbits from these measurements, but CFG seems to have devised a valid method 200 years ago. Try to find it.
 
For a fairly extensive description of the process I can recommend [1]. For an introduction I would recommend that you find an astronomy textbook suitable for your level that also describes orbital determination (like Gauss method). There is a fairly big difference between just knowing what practical observations to make in order to determine orbits, and then to derive the theory and computer code needed to make the actual calculations.

[1] Statistical Orbit Determination, Byron D. Tapley, Bob E. Schutz, George Henry Born. Elsevier Academic Press, 2004. (http://books.google.com/books?id=qePVQF9v15kC)
 

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