We show that this statistical framework correctly estimates the ab... ▽ More We extend the statistical analysis of Lissauer et al. (2012, ApJ 750, 112), which demonstrates that the overwhelming majority of Kepler candidate multiple transiting systems (multis) represent true transiting planets, and develop therefrom a procedure to validate large
numbers of planet candidates in multis as bona fide exoplanets.
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.
The findings increase
the number of planet candidates identified so far by Kepler to 1,235.
Not exact matches
«This gives astronomers a statistically sound population
of planet candidates to accurately determine the
number of small, possibly rocky
planets like Earth in our Milky Way galaxy.»
A large
number of exoplanets and
planet candidates are known, but the Earth - size exoplanets in Earth - like orbits still reside in an open part
of discovery space.
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.
This brings the total
number of KOIs and
planet... ▽ More \ We present the sixth catalog
of Kepler
candidate planets based on nearly 4 years
of high precision photometry.
The results include new asteroseismic solutions for four host stars with confirmed
planets (Kepler - 4, Kepler - 14, Kepler - 23 and Kepler - 25) and increase the total
number of Kepler host stars with asteroseismic solutions... ▽ More We have used asteroseismology to determine fundamental properties for 66 Kepler
planet -
candidate host stars, with typical uncertainties
of 3 % and 7 % in radius and mass, respectively.
Based on Kepler observations conducted from May 2009 to September 2010, the
planet findings show a dramatic increase in the
numbers of smaller - size
planet candidates, where Earth - size and super-Earth-size
candidates have increased in
number by more than 204 and 136 percent, respectively, since the last Kepler announcement in February 2011.