Extrasolar planet | List of extrasolar planets | |
---|---|---|
Parent star | ||
Star | Lupus-TR-3 | |
Constellation | Lupus | |
Right ascension | (α) | 15h 30m 18.67s |
Declination | (δ) | −42° 58′ 41.5″ |
Distance | 8950 ly (2744 pc) |
|
Spectral type | K1V | |
Orbital elements | ||
Semimajor axis | (a) | 0.0464 ± 0.0007 AU |
Eccentricity | (e) | 0 |
Orbital period | (P) | 3.91405 ± 4e-5 d |
Inclination | (i) | 88.3+1.3-0.8° |
Time of periastron | (T0) | 2453887.0818 JD |
Semi-amplitude | (K) | 114 ± 25 m/s |
Physical characteristics | ||
Mass | (m) | 0.81 ± 0.18 MJ |
Radius | (r) | 0.89 ± 0.07 RJ |
Density | (ρ) | 1400 ± 400 kg m-3 |
Discovery information | ||
Discovery date | November 12, 2007 | |
Discoverer(s) | Weldrake et al. | |
Detection method | Transit | |
Discovery site | Siding Spring Observatory | |
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia |
data | |
SIMBAD | data |
Lupus-TR-3b is an extrasolar planet orbiting the star Lupus-TR-3 (a K-type main sequence star approximately 8,950 light-years away in the constellation Lupus). The planet was discovered in 2007 by personnel from the Harvard-Smithsonian Center for Astrophysics observing at the Siding Spring Observatory in Australia, by the transit method.
The planet has four-fifths the mass of Jupiter, nine-tenths the radius, and has density of 1.4 g/cm³. This planet is a typical “Hot Jupiter” as it orbits at 0.0464 AU distance from the star, taking 3.9 days to orbit. It is currently the faintest ground-based detection of a transiting planet.[1]
Media related to [//commons.wikimedia.org/wiki/Category:Lupus-TR-3_b Lupus-TR-3b] at Wikimedia Commons