2024年10月24日 · WASP-11 b is a gas giant exoplanet that orbits a K-type star. Its mass is 0.79 Jupiters, it takes 3.7 days to complete one orbit of its star, and is 0.0435 AU from its star. Its discovery was announced in 2008.

WASP-11b/HAT-P-10b or WASP-11Ab/HAT-P-10Ab [3] is an extrasolar planet discovered in 2008. The discovery was announced (under the designation WASP-11b) by press release by the SuperWASP project in April 2008 along with planets WASP-6b through to WASP-15b , however at this stage more data was needed to confirm the parameters of the planets and ...

WASP-11b/HAT-P-10b 是一颗于2008年发现的系外行星，发现结果于2008年4月由 超级广角行星搜索计划 项目的出版物公布，同时公布的发现结果还包括从WASP-6b到WASP-15b的数颗系 …

WASP-11/HAT-P-10 是一顆視星等12的 橙矮星，距離地球約400光年，位於 白羊座 [1]。 一顆質量大約是木星一半的 系外行星 WASP-11b/HAT-P-10b 被兩個系外行星搜尋計畫以凌日法獨立發現，該行星的軌道是圓形 [2][3]。 ^ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 SIMBAD query result: NAME HAT P-10 -- Star. Centre de Données astronomiques de Strasbourg. [2009-05-05]. （原始内容 存档 于2013-07-07）. ^ 2.0 2.1 West; et al.

In this paper we report the discovery of WASP-11b, a sub-Jupiter mass gas giant planet in orbit about the host star 1SWASP J030928.54+304024.7. We present the WASP discovery photometry plus higher precision optical follow-up and radial velocity measurements which taken together confirm the planetary nature of WASP-11b. 2 Observations

2008年9月26日 · WASP-11b is the third least strongly irradiated transiting exoplanet discovered to date, experiencing an incident flux F_p=1.9x10^8 erg s^{-1} cm^{-2} and having an equilibrium temperature T_eq=960+-70K.

In this paper we report the discovery of WASP-11b, a sub-Jupiter mass gas giant planet in orbit about the host star 1SWASP J030928.54+304024.7. We present the WASP discov-ery photometry plus higher precision optical follow-up andra-dial velocity measurements which taken together confirm the planetary nature of WASP-11b. 2. Observations 2.1.

A semi-Jovian planet, WASP-11b/HAT-P-10b (WASP-11 A b/HAT-P-10 A b), 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.

ExoClock - WASP-11b, check data upload to ExoClock about WASP-11b.

It is amongst the smallest, least massive and lowest luminosity stars known to harbour a transiting exoplanet. WASP-11b is the third least strongly irradiated transiting exoplanet discovered to date, experiencing an incident flux F p = 1.9×10 8 erg s-1 cm-2 and having an equilibrium temperature T_eql = 960 ± 70 K.