Selected population of
planet candidates detected by the Kepler Space Telescope.
The distribution of observed period ratios sh... ▽ More About one - third of the ~ 1200 transiting
planet candidates detected in the first four months of \ ik data are members of multiple candidate systems.
Abstract: About one - third of the ~ 1200 transiting
planet candidates detected in the first four months of \ ik data are members of multiple candidate systems.
Not exact matches
The standard approach has been to take additional observations for each
candidate to rule out possible false positive scenarios, or to
detect the
planet with a second technique.
NASA came under criticism in June when it announced that its space - based telescope Kepler had
detected 706 potential new exoplanets, but only released data for 306 of the
candidate planets.
A number of
planet candidates are three to four times larger than Jupiter, which means that Kepler most likely
detected double - star systems in which one star was passing in front of the other.
When it was first
detected and reported last year in Astrophysical Journal, Gliese 581g appeared to be the perfect
candidate for a true «Earth - like»
planet.
Several Earth - like
planets and super-Earths have been
detected in the habitable zones of their host stars and more than 2300 planetary
candidates have been announced.
On March 25, 2015, a team of astronomers using the Hubble Space Telescope revealed observations which indicate via the transit method that Alpha Centauri B may have a second
planet «c» in a hot inner orbit, just outside
planet candidate «b.» After observing Alpha Centauri B in 2013 and 2014 for a total of 40 hours, the team failed to
detect any transits involving
planet b (previously
detected using the radial velocity variations method and recently determined not to be observed edge - on in a transit orbit around Star B).
Transit signals
detected in 2013 observations indicate that planetary
candidate c could be an Earth - sized
planet with a year lasting no more than 20.4 days, putting it slightly further out than Bb but still scorchingly close to the star (Demory et al, 2015; and Jacob Aron, New Scientist, March 27, 2015).
By comparing their distribution with that of the Kepler Objects of Interest
detected during the first six quarters of operation of the spacecraft, we infer the false positive rate of Kepler and study its dependence on spectral type,
candidate planet size, and orbital period.
We present here 275
planet candidates observed during Campaigns 0 - 10 of the K2 mission that are orbiting stars brighter than 13 mag (i... ▽ More Since 2014, NASA's K2 mission has observed large portions of the ecliptic plane in search of transiting
planets and has
detected hundreds of
planet candidates.
We then compare the number of observed
planet candidates to the number of stars around which such
planets could have been
detected in order to estimate the
planet occurrence rate around cool stars.
There are 49
planet candidates around these stars, including 42
detected through transits and 7 revealed by precise Doppler measurements of the host stars.
Abstract: Since 2014, NASA's K2 mission has observed large portions of the ecliptic plane in search of transiting
planets and has
detected hundreds of
planet candidates.
Abstract: We recently used near - infrared spectroscopy to improve the characterization of 76 low - mass stars around which K2 had
detected 79
candidate transiting
planets.
The study, which took five years, only looked for
planets that orbited rather close to their parent stars (unless the
planet is very large the signal from its gravitational hug is too slight to
detect with today's technology) so this batch won't produce good
candidates for worlds with liquid surface water that might be suited for life.
These results are based on the 1,235
planets (formally «
planet candidates») from the Kepler mission that include a nearly complete set of
detected planets as small as 2 Earth radii (Re).
K2 - 27b is a warm Neptune orbiting its host star in 6.77 days and has a... ▽ More We report on Doppler observations of three transiting
planet candidates that were
detected during Campaign 1 of the K2 mission.
Astronomers have
detected more than 1,000 confirmed
planets and almost 5,000
candidates beyond our solar system, with most of them found by NASA's Kepler Space Telescope.
Abstract: We report on Doppler observations of three transiting
planet candidates that were
detected during Campaign 1 of the K2 mission.
In particular, it was shown that less than half of the
detected big transiting
planet candidates are actually there.
The smallest
planet orbits Kepler - 33, a star older and more massive than our Sun, Sol, which also had the most
detected planet candidates at five (ranging in size from 1.5 to 5 times that of Earth) in uninhabitable, hot inner orbits closer to their star than even Mercury around our Sun (NASA Kepler news release; and JPL news release).