V385 Andromedae is a variable star in the constellation Andromeda, about 360 parsecs (1,200 ly) away. It is a red giant over a hundred times larger than the sun. It has an apparent magnitude around 6.4, just about visible to the naked eye in ideal conditions. V385 Andromedae was identified as a long-period variable in 1999 from analysis of Hipparcos photometry. It was classified as a slow irregular variable, but analysis of its light curve identified a possible 36 day period. It varies by about 0.1 magnitudes.
Attributes | Values |
---|---|
rdf:type |
|
rdfs:label |
|
rdfs:comment |
|
foaf:name |
|
foaf:depiction | |
dcterms:subject | |
Wikipage page ID |
|
Wikipage revision ID |
|
Link from a Wikipage to another Wikipage |
|
Link from a Wikipage to an external page | |
sameAs | |
dbp:wikiPageUsesTemplate | |
thumbnail | |
appmag v |
|
b-v |
|
class |
|
constell | |
epoch |
|
luminosity |
|
p error |
|
parallax |
|
prop mo dec |
|
prop mo ra |
|
radius |
|
temperature |
|
type | |
variable | |
has abstract |
|