A 12-year sequence of telescope images of a star and four planets orbiting
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Unofficial Hacker News client; not affiliated with Y Combinator.
A 12-year sequence of telescope images of a star and four planets orbiting
Unofficial Hacker News client; not affiliated with Y Combinator.
ortusdux · · focus · HN ↗
<a href="https://www.jpl.nasa.gov/missions/the-roman-coronagraph-instrument/" rel="nofollow">https://www.jpl.nasa.gov/missions/the-roman-coronagraph-inst...
The Roman Coronagraph is designed to detect planets 100 million times fainter than their stars, which is 100 to 1,000 times better than existing space-based coronagraphs. The Roman Coronagraph will be capable of directly imaging reflected starlight from a planet akin to Jupiter in size, temperature, and distance from its parent star.
izend · · focus · HN ↗
lukeify · · focus · HN ↗
As long as the telescope can fit through the Starlink Pez dispenser.
alexpotato · · focus · HN ↗
B. You could have multiple panels operate as a swarm. There could be many "mirrors" that focus images on one central "collector". That would be larger than any telescope that needs to be shipped as one unit e.g. James-Webb.
grvbck · · focus · HN ↗
Is that level of precision even remotely achievable with today's technology?
My understanding is that orbital insertion accuracy is in the ±10-50 meters range, with the most advanced formation flying satellite swarms hitting 10 cm to 1 m precision between satellites with the help of optical navigation.
But the precision between the panels on a telescope like JWST is in the sub-mm range, no?
Also, I'd assume stuff like orbital decay, atmospheric drag, gravitational perturbations, and solar radiation pressure would make it difficult to maintain precision over time.
I'm sure/hopeful there's some people here at HN working on stuff like this, please fill in and correct me!