Hubbry Logo
search
search button
Sign in
Historyarrow-down
starMorearrow-down
Hubbry Logo
search
search button
Sign in
WASP-11
Community hub for the Wikipedia article
logoWikipedian hub
Welcome to the community hub built on top of the WASP-11 Wikipedia article. Here, you can discuss, collect, and organize anything related to WASP-11. The purpose of the hub is to connect people, foster deeper knowledge, and help improve the root Wikipedia article.
Add your contribution
Inside this hub
WASP-11
WASP-11
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Aries[1]
Right ascension 03h 09m 28.5434s[2]
Declination +30° 40′ 24.863″[2]
Apparent magnitude (V) 11.57 ± 0.15[3]
Characteristics
Spectral type K3V[4]
Apparent magnitude (B) 12.58 ± 0.30[3]
Apparent magnitude (V) 11.57 ± 0.15[3]
Apparent magnitude (J) 10.015 ± 0.020[5]
Apparent magnitude (H) 9.560 ± 0.019[5]
Apparent magnitude (K) 9.421 ± 0.017[5]
Variable type planetary transit[6]
Astrometry
Radial velocity (Rv)5.21±0.28[2] km/s
Proper motion (μ) RA: 3.334(68) mas/yr[2]
Dec.: −44.433(53) mas/yr[2]
Parallax (π)7.6997±0.0579 mas[2]
Distance424 ± 3 ly
(129.9 ± 1.0 pc)
Details[7]
WASP-11 A
Mass0.77±0.02[8] M
Radius0.74±0.01[8] R
Luminosity0.28±0.002[8] L
Surface gravity (log g)4.58±0.02[8] cgs
Temperature4,884±16[8] K
Metallicity [Fe/H]0.25±0.07[9] dex
Rotational velocity (v sin i)1.9±0.9[9] km/s
Age8.7±3.5[8] Gyr
WASP-11 B
Mass0.34 M
Temperature3,494±37[10] K
Other designations
HAT-P-10, TOI-4516, TIC 85593751, WASP-11, TYC 2340-1714-1, GSC 02340-01714, 2MASS J03092855+3040249[3]
Database references
SIMBADdata
Exoplanet Archivedata

WASP-11, also designated HAT-P-10, is a binary star system. The primary star is a main-sequence orange dwarf star. The secondary is an M dwarf with a projected separation of 42 AU.[10] The system is located about 424 light-years away[2] in the constellation Aries.

Planetary system

[edit]

A hot Jupiter with half Jupiter's mass, WASP-11b (or HAT-P-10b), was detected around the primary star independently by the Hungarian Automated Telescope Network and the Wide Angle Search for Planets teams, both of which used the transit method.[4][6]

The WASP-11 planetary system[11]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.532+0.020
−0.021
 MJ
0.04376+0.00071
−0.00067
3.7224793±0.0000007 <0.03 89.03±0.34° 0.990±0.022 RJ

References

[edit]
[edit]
Add your contribution
Related Hubs