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Beta Hydri

 
Wikipedia: Beta Hydri
Beta Hydri
Observation data
Epoch J2000      Equinox J2000
Constellation Hydrus
Right ascension 00h 25m 45.07s [1]
Declination –77° 15′ 15.3″ [1]
Apparent magnitude (V) 2.80
Characteristics
Spectral type G2 IV
U-B color index 0.11
B-V color index 0.61
Variable type Suspected
Astrometry
Radial velocity (Rv) 22.9 km/s
Proper motion (μ) RA: 2,219.54 ± 0.11 [1] mas/yr
Dec.: 324.09 ± 0.11 [1] mas/yr
Parallax (π) 134.07 ± 0.11[1] mas
Distance 24.33 ± 0.02 ly
(7.459 ± 0.006 pc)
Absolute magnitude (MV) 3.43
Details
Mass 1.1 M
Radius 1.9 R
Luminosity 3.53 L
Temperature 5,750 K
Metallicity 49-100%
Rotation 3.3 km/s. (~29 days)
Age 6.7 × 109 years
Other designations
Gl 19, HR 98, CD -77°15, HD 2151, LHS 6, LTT 226, GCTP 69, SAO 255670, CP(D)-77 16, FK5 11, LPM 22, LFT 43, HIP 2021.

Beta Hydri (β Hyi / β Hydri) is a star in the constellation Hydrus (Note that Hydrus is not the same as Hydra).

It is about 24.4 light years away from Earth. Beta Hydri is often studied because it might give insights on what might happen to our Sun in the next 2.5 billion years.[citation needed] It is larger and slightly more massive than the Sun.

At around 150 BC, this star was two degrees away from the southern celestial pole. It is currently the nearest relatively bright star to the southern pole.

Contents

A planetary system?

In 2002 Endl et al. inferred the possible presence of an unseen companion orbiting Beta Hydri as hinted by radial velocity linear trend with a periodicity exceeding 20 years. A substellar object with minimum mass of 4 Jupiter masses and orbital separation of roughly 8 Astronomical Units could explain the observed trend[2]. If confirmed, it would be a true Jupiter-analogue, though 4 times more massive. So far no planetary/substellar object has been certainly detected.

The Beta Hydri system[2]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(years)
Eccentricity
b (unconfirmed) ≥4 MJ 7.6 >20 0

See also

References

External links


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