HAT-P-1b - Wikipedia
HAT-P-1b is an extrasolar planet orbiting the Sun-like star HAT-P-1, also known as ADS 16402 B. HAT-P-1 is the dimmer component of the ADS 16402 binary star system. It is located roughly …
HAT-P-1b - 维基百科，自由的百科全书
HAT-P-1b是由哈佛-史密松天文物理中心的天文學家利用一個稱為HAT的自動小型望遠鏡網路所發現的，當時HAT-P-1b讓ADS 16402 B的亮度下降了0.6%。 它的軌道非常接近恆星，距離僅 …
HAT-P-1 b - Science@NASA
2024年10月24日 · HAT-P-1 b is a gas giant exoplanet that orbits a F-type star. Its mass is 0.525 Jupiters, it takes 4.5 days to complete one orbit of its star, and is 0.05561 AU from its star. Its …
HAT-P-1b - 维基百科，自由的百科全书 - zh.wikipedia.org
2014年2月9日 · HAT-P-1b是由哈佛-史密松天文物理中心的天文学家利用一个称为HAT的自动小型望远镜网络所发现的，当时HAT-P-1b让ADS 16402 B的亮度下降了0.6%。 它的轨道非常接近 …
HAT-P-1b - 維基百科，自由的百科全書 - zh.wikipedia.org
HAT-P-1b是由哈佛-史密松天文物理中心的天文學家利用一個稱為HAT的自動小型望遠鏡網絡所發現的，當時HAT-P-1b讓ADS 16402 B的亮度下降了0.6%。 它的軌道非常接近恆星，距離僅 …
Detection of Na and K in the Atmosphere of the Hot Jupiter HAT-P-1b ...
2022年10月5日 · Our new DBSP observations of HAT-P-1b have revealed a broad spectral signature around the Na line at 5.9σ, indicating the presence of a pressure-broadened line …
HAT-P-1b: A Large-Radius, Low-Density Exoplanet Transiting
2007年2月10日 · The planet, designated HAT-P-1b, appears to be at least as large in radius, and smaller in mean density, than any previously known planet.
troscopic data leads to the conclusion that this object, HAT-P-1b, is indeed a planet and has a radius comparable to that of HD 209458bandasomewhatlowermeandensity.Intheremainder
[astro-ph/0609369] HAT-P-1b: A Large-Radius, Low-Density …
2006年9月13日 · Using small automated telescopes in Arizona and Hawaii, the HATNet project has detected an object transiting one member of the double star system ADS 16402 AB. This …
HAT-P-1b: A Large-Radius, Low-Density Exoplanet Transiting One Member ...
The planet, designated HAT-P-1b, appears to be at least as large in radius, and smaller in mean density, than any previously known planet. Based in part on data collected at the Subaru …