HAT-P-27, also known as WASP-40, is the primary of a binary star system about 659 light-years away. It is a G-type main-sequence star. The star's age is similar to the Sun's at 4.4 billion years. [2] HAT-P-27 is enriched in heavy elements, having …

2024年10月24日 · HAT-P-27 b is a gas giant exoplanet that orbits a G-type star. Its mass is 0.62 Jupiters, it takes 3 days to complete one orbit of its star, and is 0.04 AU from its star. Its discovery was announced in 2011.

Meet people from all over the country (or world). Be as anonymous as you need or want to be. Naughty or nice? That's between you and your chat partner. And Santa's list. Got it? Good!

Stellar Companions Beyond 50 au Might Facilitate Giant Planet Formation, but Most are Unlikely to Cause Kozai-Lidov Migration. New and updated stellar parameters for 90 transit hosts. The effect of the surface gravity.

2025年1月17日 · NASA Cameras on Blue Ghost Capture First-of-its-Kind Moon Landing Footage

2024年10月10日 · HAT-P-27 b is a Confirmed extrasolar planet (exoplanet) that orbits the star Wasp 40 in the constellation of Virgo

Yellow star HAT-P-27 is located 659 light years away from the Sun. It is a single star of spectral class G8, that has 95 % of solar mass. There are multiple known exoplanets in this system. Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).

The planetary system HAT-P-27 hosts at least one planet. This list shows all planetary and stellar components in the system. It gives a quick overview of the hierarchical architecture. This table lists all planets in the system HAT-P-27. This table lists all stars in the system HAT-P-27.

Exoplanet HAT-P-27 b orbits star HAT-P-27 that lies 659 light years away from the Sun. It weighs about 209.8 Earth masses and orbits its star much closer than Earth orbits Sun.

2024年10月24日 · HATS-27 b is a gas giant exoplanet that orbits a F-type star. Its mass is 0.53 Jupiters, it takes 4.6 days to complete one orbit of its star, and is 0.0611 AU from its star. Its discovery was announced in 2016.