Collision Avoidance Challenge(kelvins.esa.int)
kelvins.esa.int
Collision Avoidance Challenge
https://kelvins.esa.int/collision-avoidance-challenge/home/
6 comments
F10.7 is the measured solar power flux at 10.7 cm wavelength. It is measured all over the world but primarily from Penticton observatory in Canada.
The largest source of uncertainty in orbit propagation for satellites in Low-Earth Orbit (LEO) is atmospheric drag. Solar activity directly effects the density of the atmosphere. It is an input to many atmospheric models which are used when propagating orbits. Which is central to all conjunction assessments (predicting where objects will be in case they might come too close).
The largest source of uncertainty in orbit propagation for satellites in Low-Earth Orbit (LEO) is atmospheric drag. Solar activity directly effects the density of the atmosphere. It is an input to many atmospheric models which are used when propagating orbits. Which is central to all conjunction assessments (predicting where objects will be in case they might come too close).
The sun heats the object and causes it to emit vapor, it emits more vapor on the side facing the sun, these emissions have a measurable affect on the orbit.
See the section on 2l/Borisov
https://en.wikipedia.org/wiki/Comet#Long_period
See the section on 2l/Borisov
https://en.wikipedia.org/wiki/Comet#Long_period
Are there any more past or present challenges like these?
Timeline at the top of the page seems to indicate this opened a few days ago and runs through December 2019?
Clicking on "Competitions" in the site header reveals the past competitions?
F10: 10.7 cm radio flux index [10−22 W/(m2 Hz)]
It seems to be some sun radio activity index, but why is it relevant to collisions?