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 present here 275
planet candidates observed during Campaigns 0 - 10 of the K2 mission that are orbiting stars brighter than 13 mag (in Kepler band) and for which we have obtained high - resolution spectra (R = 44,000).
Not exact matches
In a few other cases a
candidate planet had been
observed near a star but had not been proved to follow a
planet - like orbit.
Since first
observing a
planet orbiting a star other than our sun in 1992, astronomers have made definitive sightings of about 1000 «exoplanets» and have identified a further 3000 to 4000
candidate exoplanets.
However, Kepler
observed hundreds of stars that have multiple
planet candidates.
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).
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.
Comparing single -
planet candidate KOIs to multi-
planet candidate KOIs, we find an
observed false positive fraction due to contamination of 16 % and 2.4 % respectively, bolstering the existing evidence that multi-
planet KOIs are significantly less likely to be false positives.
Since a
planet's radius and equilibrium temperature depends on the parameters of its host star, our study provides more precise planetary parameters for
planets and
candidates orbiting late - type stars
observed with K2.
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.
Since the Kepler mission began in 2009, a total of 4,034
candidates and 2,335 confirmed
planets have been spotted in the small slice of the sky the telescope
observes, which is centered on the Cygnus constellation.
By
observing slight dips in the light from distant stars — which correspond to
planets «transiting» between their host stars and the telescope's lens — Kepler has discovered 135 confirmed
planets and 3,548
planet candidates.
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.
Before we can use James Webb to really
observe candidate exoplanets and study their atmospheres, we first need to confirm the
planets are real — that what we think are
planets are not false positives caused, for instance, by stellar activity.