Kepler-62b

Kepler-62b

Discovery
Discovered by	Boruckiet al.
Discovery site	Kepler Space Observatory
Discovery date	18 April 2013
Detection method	Transit(Kepler Mission)
Orbital characteristics
Semi-major axis	0.0553 ± 0.0005AU
Eccentricity	~0
Orbital period (sidereal)	5.714932 ± 0.000009d
Inclination	89.2 ± 0.4
Star	Kepler-62(KOI-701)
Physical characteristics
Mean radius	1.31 ± 0.04R🜨
Mass	<9ME
Temperature	Teq:750 K (477 °C; 890 °F)

Kepler-62b(also known by its Kepler Object of Interest designationKOI-701.02) is the innermost and the second smallestdiscoveredexoplanetorbiting the starKepler-62,with a diameter roughly 30% larger thanEarth.It was found using thetransit method,in which the dimming effect that a planet causes as it crosses in front of its star is measured. It is likely to have an equilibrium temperature slightly higher than the surface temperature ofVenus(around 750 K (477 °C; 890 °F)), high enough to melt some types of metal.Itsstellar fluxis 70 ± 9 times Earth's.

Physical characteristics

Mass, radius and temperature

Kepler-62b is asuper-Earth,an exoplanet with a radius and mass bigger than Earth but smaller than that of the ice giantsNeptuneandUranus.It has anequilibrium temperatureof 750 K (477 °C; 890 °F). This is hot enough to melt some types of metal. It has a radius of 1.3R_🜨,placing it below the estimated radius of ≤1.6R_🜨where it would otherwise be amini-Neptunewith a volatile composition, with no solid surface.However, the mass is currently not known, estimates place an upper limit of <9M_E,the actual mass is expected to be significantly lower than this.

Host star

Main article:Kepler-62

The planet orbits a (K-type)starnamedKepler-62,orbited by a total of five planets, of whichKepler-62fhas the lengthiest orbital period.The star has a mass of 0.69M_☉and a radius of 0.64R_☉.It has a temperature of 4925Kand is 7 billion years old.In comparison, theSunis 4.6 billion years oldand has a surface temperature of 5778 K.

The star'sapparent magnitude,or how bright it appears from Earth's perspective, is 13.65. Therefore, it is too dim to be seen with the naked eye.

Orbit

Kepler-62b orbits its host star with an orbital period of 5 days at a distance of about 0.05AU(compared to the same distance asMercuryfrom the Sun, which is about 0.38AU). It receives 70 times as muchsunlightthan Earth does from the Sun.

Discovery

In 2009,NASA'sKeplerspacecraft was completing observing stars on itsphotometer,the instrument it uses to detecttransitevents, in which a planet crosses in front of and dims its host star for a brief and roughly regular period of time. In this last test, Kepler observed50000stars in theKepler Input Catalog,including Kepler-62; the preliminary light curves were sent to the Kepler science team for analysis, who chose obvious planetary companions from the bunch for follow-up at observatories. Observations for the potential exoplanet candidates took place between 13 May 2009 and 17 March 2012. After observing the respective transits, which for Kepler-62b occurred roughly every 5 days (its orbital period), it was eventually concluded that a planetary body was responsible for the periodic 5-day transits. The discovery, along with the planetary system of the starKepler-69were announced on April 18, 2013.