Enif (Epsilon Pegasi)
The brightest star in the constellation Pegasus.
Its name comes from the Arabic for "the nose" and refers to the muzzle of
the winged horse. Enif is an orange supergiant K
star, big enough, if put in place of the Sun, to stretch halfway to
the orbit of Venus. It seems to be part of
a family of three similar supergiants that also includes the Alpha and Beta
stars of nearby Aquarius, Sadalmelik and Sadalsuud. The stellar trio, all
at roughly the same luminosity and distance (Sadalmelik at 760 light-years,
Sadalsuud at 610) may have been born together in the same extended group
and. over the past 15 million years or so, have drifted well over 100 light-years
apart. Most odd about Enif is its possible erratic and violent behavior.
In 1972, an observer in Florida reported Enif to be as bright as Altair
– five times brighter than normal – after which it faded. For
over 10 minutes it appeared to pop some kind of enormous flare, one vastly
brighter than those often seen on the Sun. Such events are rare –
only two dozen or so are known – and not well documented, nor is there
any theory for them.
| visual magnitude |
2.38 |
| absolute magnitude |
-4.19 |
| spectral type |
K2Ib |
| surface temperature |
4,460 K |
| luminosity |
6,700 Lsun |
| radius |
150 Rsun |
| mass |
10 Msun |
| distance |
673 light-years |
| position |
R.A. 21h 44m 11.2s,
Dec. +09° 52' 30" |
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