I want to find the true anomaly of satellites in elliptic orbits. How can I do that with following information about elliptic orbit:
Altitude, km 543.8832
Period, sec 6114
Eccentricity 0.0727
Semi-major axis, km 7227.5
Inclination, deg 81.0192
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Sign up to join this communityI want to find the true anomaly of satellites in elliptic orbits. How can I do that with following information about elliptic orbit:
Altitude, km 543.8832
Period, sec 6114
Eccentricity 0.0727
Semi-major axis, km 7227.5
Inclination, deg 81.0192
Given the information you've provided, you can't fully determine the orbital elements but you can have a bit of a guess. For a Kepler orbit:
$$r(\theta) = {a(1-e^2) \over 1 + e \cos \theta}$$
You've given us $a$ and $e$, but converting the altitude you've supplied to an orbital radius is potentially a bit more of a faff. With a suitable model of Earth's shape and the inclination of the orbit (which you do know, at least) you might be able to manage it, but I'm not going to try.
Obviously you can rearrange the above equation to give you $\cos \theta = {a(1-e^2) \over er} - \frac{1}{e}$, and if Earth was perfectly spherical and had a nice tractable radius like 6378.1km (which it wouldn't) you could get out a true anomaly of ±57.9° but you couldn't tell which was the true true anomaly, nor which direction the orbit was in. There are some chunky error bars on that number due to the shape of the Earth that I'm not going to try and quantify.
To fully constrain an orbit you do need 6 elements, and you've supplied 5-ish (more like 4-and-a-bit, given Earth's frustrating wrinkliness and non-sphericity). Without additional information, you can't do much better.
There's not enough information in your list to compute the true anomaly. The true anomaly reflects an angular position of an object along its orbit. The parameters in the question define the shape of the orbit, but not a location along the orbit.