HD 100777

HD 100777 / Sagarmatha
Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 11h 35m 51.52322s
Declination −04° 45 20.5046
Apparent magnitude (V) 8.42
Characteristics
Spectral type G8V
B−V color index 0.76±0.02
Astrometry
Radial velocity (Rv)1.10±0.14 km/s
Proper motion (μ) RA: −11.535 mas/yr
Dec.: 35.586 mas/yr
Parallax (π)20.1590±0.0285 mas
Distance161.8 ± 0.2 ly
(49.61 ± 0.07 pc)
Absolute magnitude (MV)4.95
Details
Mass1.032+0.042
−0.045
 M
Radius1.033+0.021
−0.018
 R
Luminosity0.946+0.003
−0.004
 L
Surface gravity (log g)4.402±0.265 cgs
Temperature5,611±42 K
Metallicity [Fe/H]0.330±0.096 dex
Rotational velocity (v sin i)1.676±0.230 km/s
Age4.78+2.20
−2.14
 Gyr
Other designations
Sagarmatha, BD–03°3147, HD 100777, HIP 56572, SAO 138288, TYC 4933-678-1, 2MASS J11355152-0445204
Database references
SIMBADdata
Exoplanet Archivedata

HD 100777 is a single star with a planetary companion in the equatorial constellation of Leo. With an apparent visual magnitude of 8.42 it is too faint to be viewed with the naked eye, although the absolute magnitude of 4.81 indicates it could be seen if it were just 33 ly (10 pc) away. The distance to the star is approximately 162 light-years based on parallax measurements.

The International Astronomical Union held the NameExoWorlds campaign in 2019. Nepal named the star Sagarmatha, the Nepali name of Mount Everest, and the exoplanet revolving it was named as Laligurans, the Nepali name of the flower Rhododendron.

This is an ordinary G-type main-sequence star with a stellar classification of G8V. It has a similar mass, size, and luminosity to the Sun. The star is roughly five billion years old with an inactive chromosphere and is spinning with a projected rotational velocity of 1.7 km/s. A 2015 survey ruled out the existence of any additional stellar companions at projected distances from 18 to 369 astronomical units.