Groombridge 34
![Sky map](http://upload.wikimedia.org/wikipedia/commons/thumb/e/e4/Jupiter_and_moon.png/20px-Jupiter_and_moon.png)
![]() Ultraviolet band light curves for GX Andromedae, with flares marked by red arrows. Adapted from Pettersen and Griffin (1980)[1] | ||
Observation data Epoch J2000 Equinox J2000 | ||
---|---|---|
Constellation | Andromeda | |
Groombridge 34 A | ||
Right ascension | 00h 18m 22.88498s[2] | |
Declination | +44° 01′ 22.6380″[2] | |
Apparent magnitude (V) | 8.119[3] | |
Groombridge 34 B | ||
Right ascension | 00h 18m 25.82514s[4] | |
Declination | +44° 01′ 38.0924″[4] | |
Apparent magnitude (V) | 11.007[3] | |
Characteristics | ||
Spectral type | M1.4V + M4.1V[3] | |
U−B color index | +1.24/+1.40[5] | |
B−V color index | +1.56/+1.80[5] | |
Variable type | Flare stars | |
Periastron epoch (T) | 7140+560 −140 | |
Details | ||
Groombridge 34 A | ||
Gyr | ||
Database references | ||
SIMBAD | GJ 15 A | |
GJ 15 Ab | ||
GJ 15 B | ||
ARICNS | GJ 15 A | |
GJ 15 B | ||
Location of Groombridge 34 in the constellation Andromeda |
Groombridge 34 is a
Both components are small, dim
The star system has a relatively high proper motion of 2.9
GX Andromedae
The more massive and luminous component of the pair has the
GQ Andromedae
The smaller companion bears the variable star name GQ Andromedae. It is a red dwarf main sequence star that undergoes flare events like the primary; it has a spectral type M4.1,[3] so it also has a lower effective temperature.
Planetary system
In August 2014, a planet orbiting around Groombridge 34 A was reported.
Using the
This discrepancy was later reconciled with new HIRES observations, covering a longer span of time, where both planets were recovered, constraining their minimum mass to 3.03 ME for Groombridge 34 Ab and 36 ME for Groombridge Ac. Their orbital periods are 11.4 and approximately 7,600 days, respectively. To date, this is the fourth-closest confirmed multi-planet system to the Sun, hosting the longest-period Neptune-mass exoplanet discovered so far.[7]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥3.03+0.46 −0.44 M🜨 |
0.072+0.003 −0.004 |
11.4407+0.0017 −0.0016 |
0.094+0.091 −0.065 |
— | — |
c | ≥36+25 −18 M🜨 |
5.4+1.0 −0.9 |
~7,600 | 0.27+0.28 −0.19 |
— | — |
See also
- List of nearest stars and brown dwarfs
References
- Bibcode:1980Obs...100..198P. Retrieved 30 October 2022.
- ^ S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ S2CID 19269312, 64.
- ^ S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ Bibcode:1986EgUBV........0M.
- ^ S2CID 51814894.
- ^ S2CID 54990041.
- ^ S2CID 235435757. 40.
- ^ S2CID 44208180.
- ^ "V* GX And". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2016-02-09.
{{cite web}}
: CS1 maint: postscript (link) - ^ Groombridge, Stephen (1838), Airy, George Biddell (ed.), A Catalogue of Circumpolar Stars, J. Murray, p. 2.
- Bibcode:1990A&AS...85..971P.
- ^ S2CID 59039482. A35.
- S2CID 73564680.
- S2CID 17361592, 51.
- S2CID 119340839.