
Explore the Surface - Kepler 186f - Exoplanet Exploration
Kepler-186f is the first Earth-size planet discovered in the potentially 'habitable zone' around another star, where liquid water could exist on the planet's surface.
NASA's Hubble captures blistering pitch-black planet – Exoplanet ...
The oddball exoplanet, called WASP-12b, is one of a class of so-called "hot Jupiters," gigantic, gaseous planets that orbit very close to their host star and are heated to extreme temperatures. The planet's …
Exoplanet Program: ExoPAG News and Announcements - Archive 2020
Dec 31, 2022 · NASA’s Exoplanet Exploration Program, the search for planets and life beyond our solar system.
Explore the Surface - TRAPPIST-1d - Exoplanet Exploration
Some 40 light-years from Earth, a planet called TRAPPIST-1d offers a heart-stopping view: brilliant objects in a red sky, looming like larger and smaller versions of our own moon.
NASA’s Nexus for Exoplanet System Science: Working Together to Find Life in the Universe (New!) NExSS Leadership: Ofer Cohen, Hilairy Hartnett, Jessica Noviello, Linda Sohl, and Rob Zellem
J1407b: Super-Saturn - NASA Science - Exoplanet Exploration
Jan 26, 2015 · Artist’s conception of the extrasolar ring system circling the young giant planet or brown dwarf J1407b. The rings are shown eclipsing the young sun-like star J1407, as they would have …
Exoplanet observaPons have played a major role in HST’s science program over the last decade. Over the years, the proposal pressure for exoplanet observaPons has increased significantly in proporPon …
Exoplanet Program: NASA-NSF Ground-based Support for Exoplanet ...
NASA’s Exoplanet Exploration Program, the search for planets and life beyond our solar system.
Unveiling Rogue Planets With NASA's Roman Space Telescope – …
New simulations show that NASA’s Nancy Grace Roman Space Telescope will be able to reveal myriad rogue planets – freely floating bodies that drift through our galaxy untethered to a star. Studying …
The ExEP technology goals are driven by and focused on enabling the science capability to directly image and spectrally characterize exo-earths in the HZ of Sun-like stars and beyond.