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Epsilon Reticuli - Wikipedia, the free encyclopedia

Epsilon Reticuli

From Wikipedia, the free encyclopedia

Epsilon Reticuli (A / B)
Observation data
Epoch J2000
Constellation
(pronunciation)
Reticulum
Right ascension 4h 16m 29.03s
Declination -59° 18′ 07.76″
Apparent magnitude (V) 4.44 / 12.5
Characteristics
Spectral type K2IVa / D
Astrometry
Distance 59.45 ly (18.23 pc)
Other designations
HR 1355, HD 27442, HIP 19921
Database references
SIMBAD data

Epsilon Reticuli is a binary system approximately 59 light-years away in the constellation of Reticulum. The primary star is an orange subgiant star, while the secondary star is a white dwarf star. The primary star should be easily visible without optical aid under dark skies in southern hemisphere. As of 2000, an extrasolar planet has been confirmed to be orbiting the primary star in the system.

Contents

[edit] Star system

The primary star, Epsilon Reticuli A, is an orange subgiant 20% more massive than our Sun. Being a subgiant it is ceasing or has already ceased fusing hydrogen in its core. Soon the star will swell up and become a red giant. Despite its advanced stage, it cannot be much older than the Sun.

The companion star, Epsilon Reticuli B, is a white dwarf star located around 240 AU from Epsilon Reticuli A. It has a surface temperature between 9000 and 17000 K.

[edit] Planetary system

The inner solar system superimposed behind the orbits of the planet Epsilon Reticuli b (and several others).
The inner solar system superimposed behind the orbits of the planet Epsilon Reticuli b (and several others).

On December 11, 2000, a team of astronomers announced the discovery of a planet Epsilon Reticuli b. With a minimum mass of 1.17 that of Jupiter and a similar radius, the planet moves around Epsilon Reticuli with an average separation of 1.16 AUs. The eccentricity of the planet is extremely low (at 0.06), and orbits around the star every 418 days (or 1.13 years).

The Epsilon Reticuli system
Planet
(in order from star)
Mass
(MJ)
Orbital period
(days)
Semimajor axis
(AU)
Eccentricity
b >1.56±0.14 428.1±1.1 1.271±0.073 0.060±0.043

[edit] References

[edit] External links



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