WASP-35
Sign in to saveAlso known as BD-06 1077
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.
Astronomical data · SIMBAD
- Object type
- *
- Distance
- 660 light-years
- Redshift
- z = 0.00005657407085846167
- Coordinates
- RA 76.0818° · Dec -6.2298°
View on SIMBAD →
via SIMBAD · CDS Strasbourg
Wikidata facts
- Distance from Earth
- 203.388
- Radius
- 1.1285342
Show 13 more facts
- effective temperature
- 5967
- metallicity
- -0.301
- catalog code
- TIC 43647325
- apparent magnitude
- 10.854834
- parallax
- 4.944
- radial velocity
- 19.44
- surface gravity
- 19700
- luminosity
- 1.3941189
- right ascension component of proper motion
- 20.758
- declination component of proper motion
- 10.963
- age estimated by a dating method
- 5.0
- right ascension
- 76.08180133098
- declination
- -6.22982727383
Sources (1)
via Wikidata · CC0
~1 min read
Article
2 sectionsContents
- Planetary system
- References
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 .
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