KELT-10

KELT-10 is a star in the constellation Telescopium. It was discovered by KELT, and the first star discovered by KELT-South.[3]

KELT-10
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Telescopium
Right ascension 18h 58m 11.91s[1]
Declination −47° 00 11.91[1]
Apparent magnitude (V) +9.69
Characteristics
Spectral type G0V[1]
B−V color index +0.63[2]
Astrometry
Absolute magnitude (MV)+4.3
Details
Mass1.07[1] M
Radius1.16[1] R
Luminosity0.16[1] L
Surface gravity (log g)4.34[1] cgs
Temperature5,883±406[1] K
Rotational velocity (v sin i)330 km/s
Age4.5[1] Gyr
Other designations
KELT-10
Database references
SIMBADdata

Physical properties

KELT-10 is a yellow dwarf very similar to the Sun, but 7% more massive and has 1.16 times the radius. It is also hotter, with a temperature of 5883 K, while the Sun has a temperature of 5778 K due to its spectral class. The (V) in spectral class, states that it is in the main sequence. The star is also slightly younger, with an age of 4.5 billion years.

Planetary systems

In 2015, a hot Jupiter was discovered by KELT.

The KELT-10 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.68±0.01 MJ 0.0525 4.17 88.61°° 1.14 RJ

References

  1. "Exoplanet Archive". exoplanetarchive.ipac.caltech.edu.
  2. http://www.isthe.com/chongo/tech/astro/HR-temp-mass-table-byhrclass.html
  3. Kuhn, Rudolf B.; Rodriguez, Joseph E.; Collins, Karen A.; Lund, Michael B.; Siverd, Robert J.; Colón, Knicole D.; Pepper, Joshua; Stassun, Keivan G.; Cargile, Phillip A.; James, David J.; Penev, Kaloyan (2016-07-11). "KELT-10b: the first transiting exoplanet from the KELT-South survey – a hot sub-Jupiter transiting a V = 10.7 early G-star". Monthly Notices of the Royal Astronomical Society. 459 (4): 4281–4298. doi:10.1093/mnras/stw880. ISSN 0035-8711.


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