The mission reached a milestone toward meeting that goal: the discovery of
its first rocky planet, Kepler - 10b.
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.
January 2011 saw the Kepler mission confirm finding
its first rocky planet, estimated at 1.4 times the size of Earth.
Abstract: Kepler - 10b was
the first rocky planet detected by the Kepler satellite and con - firmed with radial velocity follow - up observations from Keck - HIRES.
Earth, neighbors weren't
the first rocky planets in the solar system.
Earth and its neighbors aren't
the first rocky planets to circle the sun, a new study suggests.
Not exact matches
He then went on to tell us about the history of the universe from the huge explosion of matter and energy (the Big Bang) through the formation of stars and then
rocky planets on which complex chemicals were produced, leading to the synthesis of the
first molecules of life and the emergence of the plant and animal kingdoms.
The TRAPPIST telescope team
first announced in May 2016 that the star had three temperate,
rocky planets.
In January Kepler astronomers announced the discovery of the
first definitively
rocky planet outside our solar system, Kepler - 10 b.
Kepler 10b: Kepler's Calling Card Announced in January 2011, Kepler 10b was the mission's
first discovery of a small,
rocky planet, proof of the Kepler telescope's
planet - hunting prowess.
Unlike Saturn's bright rings, which are made almost entirely of ice particles, Mars's
rocky ring will be dark and largely invisible from Earth, although the cloud of orbiting Phobos bits will at
first be dense enough to cast a shadow on the Red
Planet's surface during some parts of the planet's orbit around the sun, the researcher
Planet's surface during some parts of the
planet's orbit around the sun, the researcher
planet's orbit around the sun, the researchers say.
Until then, all the known exoplanets (
planets circling other stars) were big and gaseous, but this one is probably made of
rocky materials — the
first world like ours found in an alien solar system.
This is the
first definitive
rocky planet, following in the footsteps of CoRoT7b.
The Gliese 667C system is the
first example of a system where such a low - mass star is seen to host several potentially
rocky planets in the habitable zone.
From this survey data, NASA's James Webb Space Telescope as well as large ground - based observatories will be able to further characterize the targets, making it possible for the
first time to study the masses, sizes, densities, orbits, and atmospheres of a large cohort of small
planets, including a sample of
rocky worlds in the habitable zones of their host stars.
«
First evidence of
rocky planet formation in Tatooine - like system.»
That precision is what makes Kepler - 10b the
first unquestionably
rocky planet orbiting another star, Batalha said.
It will revolutionize our knowledge of
rocky planets and will enable the
first directed search for life around sunlike stars in the next decade,» says Don Pollacco of the University of Warwick, who will lead the U.K. effort.
GJ 1132b is the
first in a new class of
rocky planets close enough to study in depth with today's technology — signalling that exoplanet studies are about to become more than mere stamp collecting.
Ever since the
first exoplanet was discovered in 1996, astronomers have been scanning the heavens for another Earth: a
rocky planet orbiting its star at just the right distance for it to harbor liquid water and thus, potentially, life.
In this scenario,
planets could form mainly from gas, without
first forming a
rocky core.
FIRST DRAFT The solar system may have once hosted several large
rocky planets close to the sun, like Kepler 11 (illustrated) does, before Jupiter swept them away.
Kepler - 10b was the
first «iron - clad proof of a
rocky planet beyond our solar system» back in 2001.
Under this model of ocean formation,
rocky planets with 0.5 to five Earth - masses are likely to form oceans within the
first 150 million years after formation.
«Most of the
planets in the
first group may be akin to the Earth, with
rocky surfaces and little to no atmospheres.
SPARCS will also be capable of «target - of - opportunity» UV observations for the
rocky planets in M dwarf HZs soon to be discovered by NASA's TESS mission, providing the needed UV context for the
first habitable
planets that JWST will characterize.
CoRoT - 7 b, the
first potential
rocky planet detected outside the Solar system, may be the remnant core of a Saturn - mass gas giant that had its atmosphere and lower gas metal layers burned off (more)
This study found that the
first three of those
planets don't have hydrogen - rich atmospheres, which also supports the idea that they're
rocky worlds.
Assuming an iron - rich
planet with an internal structure like Earth, modelling results for the
first discovered super-Earth (GJ 876 d) indicate the existence of a threshold in planetary diameter above which a super-Earth «most certainly» has a high water content (an «ocean
planet» or «water world,» where thick layers of water and pressurized ice surround a
rocky mantle and core); this threshold was found to be around 24,000 kilometers (or nearly 15,000 miles) in the particular case of GJ 876 d (Valencia et al, 2007).