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Gliese 570 - Wikipedia, the free encyclopedia

Gliese 570

From Wikipedia, the free encyclopedia

Gliese 570 A / B / C / D

GJ 570 D looking at star A (right) and BC (left)
Observation data
Epoch J2000.0
Constellation
(pronunciation)
Libra
Right ascension 14h 57m 28.0/27.2s
Declination -21° 24' 55/56"
Apparent magnitude (V) 5.64 / ? / 9.90
Characteristics
Spectral type K4V / M1V / M3V / T7V
U-B color index 1.06 /1.22 /?
B-V color index 1.11 / 1.51 / ?
Variable type not / ?
Astrometry
Radial velocity (Rv) +27.9 km/s
Proper motion (μ) RA: 1034.18 mas/yr
Dec.: -1725.60 mas/yr
Parallax (π) 169.85 ± 0.82 mas
Distance 19.2 ± 0.09 ly
(5.89 ± 0.03 pc)
Absolute magnitude (MV) 6.79 / ? / 11.05
Details
Mass 0.76 / 0.55 / 0.35 / 0.05 M
Radius 0.77 / 0.65 / ? R
Luminosity 0.16 / 0.02 / 0.003 / 3•10-6 L
Temperature 4170 / 2700 / ? K
Metallicity 102%
Rotation 48.3 days
Age ? years
Other designations
HD 131977 / 131976/ ?, BD -20°4125, LHS 387, LTT 5949, GCTP 3375.00, SAO 183040, FK5 1391, LFT 1161, LPM 551, Vys 726, ADS 9446, HIP 73184 / 73182 / ?

Gliese 570 (also known as HR 5568) is a trinary star about 19.2 light-years away in the constellation Libra. The system consists of an orange dwarf primary, a binary star set of red dwarfs, and a far out brown dwarf. The system is located southwest of Alpha Librae. It is the closest star system in Libra.

Contents

[edit] Gliese 570 A

Gliese 570 A is the primary star in the system.

[edit] Gliese 570 Ab

Gliese 570 Ab was an unconfirmed extrasolar planet orbiting Gliese 570 A. The planet was hypothesised by Martin Kürster in 1998 and retracted in 2000.[1]

[edit] Gliese 570 BC

Gliese 570 BC are a set of red dwarfs orbiting each other around the primary star. The pair orbit star A at about 190 AUs with a 2,130 year orbit and an eccentricity of 0.20[2]. Star B orbits about 0.31 AUs from the BC center and C orbits 0.48 AUs from the BC center and they orbit each other every 0.846 years.

[edit] Gliese 570 D

Gliese 570 D is the farthest object in the system and is a brown dwarf with a mass between 30 and 70 Jupiter masses (0.05±0.02 solar masses) and about 3•10-6 times the solar luminosity. Its separation from Gliese 570 A is at least 1500 AU[3].

[edit] See also

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[edit] External links


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