Not exact matches
The latest study to bolster this argument was presented earlier in the meeting
by lead author Courtney Dressing, another CfA astronomer, who measured the masses and sizes of a handful of
small transiting
planets to estimate the
rocky - to - gaseous transition zone.
Astronomers infer the presence of
small rocky objects that give rise to such
planets by detecting warm disks of dusty particles girdling young stars.
By the time Webb is operational, Clampin says, another NASA mission, the Transiting Exoplanet Survey Satellite (TESS), slated for launch in 2017, will already be producing a short list of other potentially habitable
rocky planets around nearby
small stars.
SS: TESS will do an all - sky survey to find
rocky worlds around the bright, closest M - stars [red dwarfs that are common and
smaller than the sun — and therefore more likely to reveal the shadows cast
by planets], about 500,000 stars.
According to a very rough statistical analysis, the new discovery suggests that up to one - third of all red dwarf stars in the Milky Way galaxy are accompanied
by small,
rocky planets, many of which might be in wider orbits.
Indeed, the present - day theory of
planet formation — the build up of a
rocky planet's core
by the accretion of many
small bodies — is very different from Jeans's.
Furthermore,
by knowing the mass of a
planet from radial velocity measurements and the radius of a
planet based on how much starlight it blocked, it is a simple calculation to determine a
planet's density, which can tell astronomers whether that
planet is
rocky or gaseous in nature, or whether it has a
small core and a thick atmosphere, or whether it has a large core covered in deep oceans.
Here we apply the light - curve modeling tech... ▽ More The Kepler Mission has recently announced the discovery of Kepler - 10 b, the
smallest exoplanet discovered to date and the first
rocky planet found
by the spacecraft.
Adibekyan and collaborators set out to find how the frequency of
small,
rocky planets in the habitable zone is affected
by the composition of the host star.
Called Interior Exploration using Seismic Investigations, Geodesy and Heat Transport, or InSight, this NASA mission aims to improve understanding about the formation and evolution of Mars and other
small,
rocky planets by looking beneath Mars's surface.