Extreme adaptive optics also allows
much fainter objects to be seen very close to a bright star.
So Anita Cochran of the University of Texas and her colleagues turned to the Hubble telescope's Wide Field / Planetary Camera, which can spot
much fainter objects.
Not exact matches
We train our telescopes on small patches of sky for long spells, trying to drink in as
much faint light from distant
objects as possible.
All seven mirrors combined gather less than one - hundredth as
much light as one 30 - foot - wide mirror, meaning they won't pull in the
faintest objects in the sky.
Ground - based and orbiting telescopes employ exquisitely sensitive detectors to search for
objects that are
much farther away, and
much fainter, than could have been detected just a few years ago.
Further studies showed that this
object, called B3 1715 +425, is a supermassive black hole surrounded by a galaxy
much smaller and
fainter than would be expected.
The JWST, a joint NASA / ESA / CSA venture that is due to launch in 2018, has a primary mirror (partially pictured at the top of the story) that's about five times larger than Hubble's, meaning it can resolve
much fainter signals, locating stars and other
objects that have never been seen before.
Once more massive and brighter than Gacrux and so burnt out
much faster, it is now probably a few hundred times
fainter than Sol, with 0.6 to 1.4 times its mass and less than one percent of its diameter — a very dense
object at planetary size.
The FOS examined
fainter objects than the High Resolution Spectrograph (HRS), and could study these
objects across a
much wider spectral range — from the UV (1150 Angstroms) through the visible red and the near - IR (8000 Angstroms).
Redshift is a measure of how
much the Universe has expanded since the light left a distant source and can only be determined for
faint objects with a spectrograph on a powerful large telescope such as the Keck Observatory's twin 10 - meter telescopes, the largest on Earth.
Most of the
objects you'll see in Disk Detective are
much fainter than this!
This was necessary because if the telescope were not cooled down, its own thermal radiation at infrared wavelengths would swamp the
much fainter radiation from astronomical
objects.