Shedar (Alpha Cassiopeiae)
 |
Alpha Cassiopeiae; 10"x4" field, ISO 400 Meade LX-90.
Credit: Kevin Muenzler, Eagle Creek Observatory
|
An orange giant K star and normally the brightest
star in the constellation Cassiopeiae, although
it is occasionally well surpassed by the strange variable Gamma
Cassiopeiae. Its name (also spelled Schedar, Shadar, or Shedir) comes
from the Arabic for "breast," and refers to the position of the star in
the ancient Queen.
Along with Hamal in Aries, Shedar has the
distinction of being one of the first two stars beyond the Sun whose limb
darkening has been directly observed. Though only 100 to 200 million
years old, it has already left the main sequence, having ceased core hydrogen
fusion. Shedar also hides a mystery because various 19th-century astronomers
claimed it could fade to mid-third magnitude. It is still called a variable
in most listings despite the fact that since the advent of permanent photographic
and electronic recording, it has shone steadily.
| visual magnitude |
2.24 |
| absolute magnitude |
-1.99 |
| surface temperature |
4,530 K |
| spectral type |
KIIIa |
| luminosity |
855 Lsun |
| radius |
42 Rsun |
| mass |
4 to 5 Msun |
| distance |
229 light-years |
| position |
R.A. 00h 40m 30.5s,
Dec. +56° 32' 14.5" |
| other designations |
18 Cassiopeiae, HR 168, BD+55°139,
HD 3712, SAO 21609, FK5 21,
HIP 3179, GC 792, ADS 561,
CCDM J00405+5632 |
Related categories
NOTABLE
STARS VARIABLE
STARS
Also on this site: Encyclopedia
of Alternative Energy & Sustainable Living
Encyclopedia
of History
BACK TO TOP
|