New planet-hunting camera produces best-ever image of an exoplanet
news.stanford.edu
news.stanford.edu
In my opinion, we need to continue to bring the cost to Low Earth Orbit down by any means necessary, including railguns for non-human traffic. Low cost-to-orbit would dramatically speed up dozens of things, exo-planet imaging among them.
As much as I love human space travel and robotic exploration, I have to admit that exoplanet research and imaging is really where all the exciting stuff is going to happen. How much longer until we have an image of another Earth? Wonder what a space-based astronomical interferometer about the width of the solar system could image? And that's what? A 10-20B project? Imagine the change in the public's imagination a series of images of the countless other planets in the galaxy would bring.
For a space-based interferometer mission, eLISA is a non-optical interferometer (for gravitatinal waves) with 1e6 km arms with a budgeted cost of 1.3B Euro. An interferometer needs to control spacing by a fraction of a wavelength, but for gravitational waves that's like 1e9 m. Optical light is 1e-7m. That's 18 orders of magnitude higher precision over a proposed 3 orders of magnitude larger baseline.
I think it's fair to say the cost of such a mission would be "out of this world", because we have no idea how to build it, and it's not the launch cost to LEO that's the problem.
James Webb Space Telescope won't be in LEO, they'll fly it to the L2 Lagrange point: http://en.wikipedia.org/wiki/James_Webb_Space_Telescope#Orbi...
There is no basis to compare the hard technology in JWST to the hard technology in a space interferometer. They are two very different beasts.
Could explain what you're saying here better? The LISA satellites will making measurements of changes in the million km distances between each other to an accuracy below 20 picometers.
I wonder if we can apply Moore's law to this? Every 1.5 year the number of pixels doubles. So in 10 years it will be 3600 pixels, an in 20 years 360k. Another 10 and the resolution needs to be so high that you'd have to fly to it to take the picture :)
http://en.wikipedia.org/wiki/Thin_disk
Star ages can be estimated by their composition (older stars contain more helium), color (bluer stars live far shorter than redder stars), brightness for their given color (older stars burn brighter), activity (younger stars are more active, they flare more) and if they contain protoplanetary disks (a feature of very young stars).
Astronomers also use the HR diagram: http://en.wikipedia.org/wiki/Hertzsprung%E2%80%93Russell_dia...
Having a good measure of distance is important and there are various ways to determine that: http://en.wikipedia.org/wiki/Cosmic_distance_ladder