Not exact matches
Taking an
optical image of distant
planets is tough because the bright light from their stars drowns them out.
The first Terrestrial
Planet Finder mission will take optical images of nearby stars and essentially put a thumb over the star itself to block the light and see the dim p
Planet Finder mission will take
optical images of nearby stars and essentially put a thumb over the star itself to block the light and see the dim
planetplanet.
And in the future, a technique called
optical interferometry, which links together the observations
of more than one telescope, might make it possible to see the multiple lensed
images produced by the
planets of another star system.
In addition, all three stars (including Proxima) were among the «Tier 1» target stars for NASA's
optical Space Interferometry Mission (SIM) to detect a
planet as small as three Earth - masses within two AUs
of its host star (and so some summary system information and
images on Stars A, B, and C are available from the SIM Teams), but the SIM project manager announced on November 8, 2010 that the mission was indefinitely postponed due to withdrawal
of NASA funding.
HDST will have unprecedented
image clarity and sensitivity in the UV and
optical and will be able to search nearby Earth - like
planets for signs
of life.
It was also selected as a «Tier 1» target star for NASA's
optical Space Interferometry Mission (SIM) to detect a
planet as small as three Earth - masses within two AUs
of its host star (and so some summary system information and
images of Epsilon Indi may still be available from the SIM Teams), but the SIM project manager announced on November 8, 2010 that the mission was indefinitely postponed due to withdrawal
of NASA funding.
To validate candidate
planets identified by K2, the researchers obtained high - resolution
images of the
planet - hosting stars from Keck Observatory's near infrared camera (NIRC2), the Gemini and Large Binocular Telescope (among others) as well as high - resolution optical spectroscopy using Keck Observatory's high resolution spectrograph (HIRES) instrument and the AUtomated Planet F
planet - hosting stars from Keck Observatory's near infrared camera (NIRC2), the Gemini and Large Binocular Telescope (among others) as well as high - resolution
optical spectroscopy using Keck Observatory's high resolution spectrograph (HIRES) instrument and the AUtomated
Planet F
Planet Finder.
To validate candidate
planets identified by K2, the researchers obtained high - resolution
images of the
planet - hosting stars as well as high - resolution
optical spectroscopy data.
It was also selected as a «Tier 1» target star for NASA's
optical Space Interferometry Mission (SIM) to detect a
planet as small as three Earth - masses within two AUs
of its host star (and so some summary system information and
images of Eta Cassiopeiae A and B may still be available from the SIM Teams), but the SIM project manager announced on November 8, 2010 that the mission was indefinitely postponed due to withdrawal
of NASA funding.