WASP-35 is a G-type main-sequence star about 660 light-years away. The star's age cannot be well constrained, but it is probably older than the Sun. WASP-35 is similar in concentration of heavy elements compared to the Sun. The star has no detectable starspot activity. An imaging survey in 2015 found no detectable stellar companions, although a spectroscopic survey in 2016 yielded a suspected red dwarf companion with a temperature of 3800±1100 K.
Attributes | Values |
---|---|
rdf:type | |
rdfs:label |
|
rdfs:comment |
|
foaf:name |
|
dct:subject | |
Wikipage page ID |
|
Wikipage revision ID |
|
Link from a Wikipage to another Wikipage | |
sameAs | |
dbp:wikiPageUsesTemplate |
|
age gyr |
|
appmag v |
|
constell | |
eccentricity |
|
epoch |
|
exoplanet | |
gravity |
|
inclination |
|
mass |
|
metal fe |
|
p error |
|
parallax |
|
period |
|
prop mo dec |
|
prop mo ra |
|
radial v |
|
radius |
|
rotational velocity |
|
semimajor |
|
temperature |
|
has abstract |
|
prov:wasDerivedFrom | |
page length (characters) of wiki page |
|
foaf:isPrimaryTopicOf | |
is Link from a Wikipage to another Wikipage of | |
is Wikipage redirect of | |
is foaf:primaryTopic of |