Not exact matches
Many of the cluster stars are
fainter than those normally targeted for exoplanet searches and trying to
detect the weak signal from possible
planets pushed HARPS to the limit.
Previous sky surveys with ground - based telescopes have mainly
detected giant
planets, while NASA's Kepler observatory has uncovered the existence of many smaller exoplanets, but their host stars are
faint and difficult to study.
«We focused on red - dwarf stars, which are smaller and
fainter than our Sun, since we expect any biomarker signals from
planets orbiting such stars to be easier to
detect.»
Planets are so
faint and tiny compared to their host stars that it is remarkable we can
detect them at all, let alone study their atmospheres.
It is the first
planet detected by the Gemini Planet Imager, or GPI, which was designed to discover and analyze faint, young planets orbiting bright, nearby
planet detected by the Gemini
Planet Imager, or GPI, which was designed to discover and analyze faint, young planets orbiting bright, nearby
Planet Imager, or GPI, which was designed to discover and analyze
faint, young
planets orbiting bright, nearby stars.
While NASA's Kepler space observatory has discovered thousands of
planets, it does so indirectly by
detecting a loss of starlight as a
planet passes in front of its star, the Gemini Planet Imager was designed specifically for discovering and analyzing faint, young planets orbiting bright
planet passes in front of its star, the Gemini
Planet Imager was designed specifically for discovering and analyzing faint, young planets orbiting bright
Planet Imager was designed specifically for discovering and analyzing
faint, young
planets orbiting bright stars.
The findings were headed by Bruce Macintosh, a professor of physics at Stanford University, and show the new
planet, 51 Eridani b, is one million times
fainter than its parent star and shows the strongest methane signature ever
detected on an alien
planet, which should yield additional clues as to how the
planet formed.
Because
planets are much
fainter than the stars they orbit, extrasolar
planets are extremely difficult to
detect directly.
While NASA's Wide - field Infrared Survey Explorer (WISE) failed to the tell - tale warmth of gas giants like Saturn within 10,000 AUs and larger than Jupiter objects out to 26,000 AUs (NASA / JPL news release), an icy «super-Earth», would have been too cold and
faint for WISE to
detect — even if the hypothesized
planet has a small internal heat source and absorbs some sunlight.