
#1
Feb2211, 03:09 AM

P: 1

Dear all,
I'm new here and I'm sorry if my problem has already been discussed anywhere else. I have some problems in determining the magnitude of space debris as a function of their dimension and distance. I have to find the visual absolute magnitude of a 30 cm diameter debris, at 36000 km and with an albedo of 0.2. As a reference, I have taken the vega V flux above the atmosfere, 8.8E5 phot/cm2/s. If I start taking into account the photon flux from 470 to 700 nm, and I consider a Lambertian surface with a phase angle of 0 for simplicity, I can find the reflected flux of photons, phot/cm2/s. Nevertheless, this flux is independent from the dimension of the debris, but it depends only on the phase angle and the albedo of the debris. When I try to consider the dimension of the object, and multiply the photon flux with the surface of the debris, I find the number of the reflected photons, express in phot/s. How can I relate this number to the absolute magnitude? Thank you a lot 


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