EF Eridani

From Infogalactic: the planetary knowledge core
Jump to: navigation, search
EF Eridani

Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Eridanus
Right ascension 03h 14m 13.03s[1]
Declination −22° 35′ 41.4″[1]
Apparent magnitude (V) 14.5–17.3[2]
Characteristics
Variable type E+XM[2]
Astrometry
Radial velocity (Rv) 70[1] km/s
Distance 300[3] ly
Other designations
GSC 6439.00120, X 03116-227[2]
Database references
SIMBAD data

EF Eridani (abbreviated EF Eri, sometimes incorrectly referred to as EF Eridanus) is a variable star of the type known as polars, AM Herculis stars, or magnetic cataclysmic variable stars. Historically it has varied between apparent magnitudes 14.5 and 17.3, although since 1995 it has generally remained at the lower limit. The star system consists of a white dwarf with a substellar massed former star in orbit.

EF Eridani B

The substellar mass in orbit around the white dwarf is a star which lost all of its gas to the white dwarf, except what remains, a 0.05 solar mass (M) ball, which is too small to continue fusion, and does not have the composition of a super-planet, brown dwarf, or white dwarf. There is no category for such a stellar remnant.[4]

It is theorized that 500 million years ago, the white dwarf started to cannibalize its partner, when they were separated by 7 million km. As it lost mass, the regular star spiralled inward, until now they are separated by a mere 700,000 km.[4]

Another former star orbits the pulsar PSR J1719-1438.[5]

See also

References

  1. 1.0 1.1 1.2 Lua error in package.lua at line 80: module 'strict' not found.
  2. 2.0 2.1 2.2 Lua error in package.lua at line 80: module 'strict' not found.
  3. Mystery Object Neither Star Nor Brown Dwarf
  4. 4.0 4.1 Lua error in package.lua at line 80: module 'strict' not found.
  5. Lua error in package.lua at line 80: module 'strict' not found.

External links


<templatestyles src="Asbox/styles.css"></templatestyles>