Q4052830
Sign in to saveWASP-26 is a G-type subgiant star about 824 light-years away in the constellation of Cetus.
In the Vinony graph
Vinony's link graph records 398 inbound references to Q4052830, and connects out to stellar classification, list of NGC objects (1–1000) and year.
Vinony files it under Binary stars, Cetus and G-type subgiants.
Vinony links it to 6 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- *
- Spectral type
- G0
- Distance
- 824 light-years
- Redshift
- z = 0.000032022665864550603
- Coordinates
- RA 4.6029° · Dec -15.2673°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Distance from Earth
- 250
- Diameter
- 1500000
- Radius
- 1.34
- Mass
- 1.12
Show 14 more facts
- catalog code
- TOI-2386
- effective temperature
- 5950
- parallax
- 3.9574
- radial velocity
- 9.60
- apparent magnitude
- 10.993513
- spectral class
- G0IV-V
- metallicity
- 0.15
- surface gravity
- 17400
- luminosity
- 1.93755
- right ascension component of proper motion
- 27.416
- declination component of proper motion
- -24.524
- right ascension
- 4.60292002534
- declination
- -15.26729882744
- age estimated by a dating method
- 6
via Wikidata · CC0
~1 min read
Encyclopedic overview
3 sectionsContents
- Star characteristics
- Planetary system
- References
WASP-26 is a G-type subgiant star about 824 light-years away in the constellation of Cetus.
== Star characteristics == WASP-26 is an old star close to leaving the main sequence and is part of a wide binary. The binary's projected separation is 3800 astronomical units, its companion star being a K-type star with an effective temperature of 4600K and a visual magnitude of 13.6. WASP-26 produces a large amount of ultraviolet light due to frequent flares, with an average ultraviolet flux close to the F7 class main-sequence star WASP-1.
Excerpted from Wikipedia’s “Q4052830” article, available under the CC BY-SA 4.0 licence.