
Is there water on an Earth-sized exoplanet? Study offers clues
TRAPPIST-1 e may have an atmosphere that could support having liquid water on the planet’s surface in the form of a global ocean or icy surface, according to new research.
Read moreCSI explores factors that determine if a planet or moon can host life and how we could find it by bringing together experts from a wide range of disciplines, from sciences, engineering to media who work together with some of the planet’s most talented students at the undergraduate, graduate and postdoctoral level.
When we explore other worlds, what once seemed the only way a planet could be turns out to be somewhere in the middle range of a vast spectrum of possibilities…
― Carl Sagan, Pale Blue Dot: A Vision of the Human Future in Space
TRAPPIST-1 e may have an atmosphere that could support having liquid water on the planet’s surface in the form of a global ocean or icy surface, according to new research.
Read moreThe award recognizes and honors outstanding communication by an active planetary scientist to the public.
Read morePhenomena common to Earth’s atmosphere can appear in the skies over some exoplanets of the “hot Jupiter” variety.
Read moreFrom designing a reversible male contraceptive to detecting life on distant ocean worlds, the latest Cornell Engineering SPROUT Awards are cultivating breakthroughs across medicine, space exploration, robotics and environmental sensing.
Read more“It’s the cutting edge of what we can achieve, with better precisions and resolutions than other instruments.”
Read moreIn a musical journey through the cosmos, the Cornell Symphony Orchestra will perform the world premiere of “Ex Terra, Ad Astra,” a new work commissioned especially for this year’s Young Person’s Concert.
Read moreIn November, we celebrated 90 years since Carl Sagan was born. On Valentine’s Day today, we celebrate 35 years since the birth of—thanks to Prof. Sagan’s persuasion—one of the greatest photographs of all time.
Read moreCornell scientists are developing a library of basalt-based spectral signatures that not only will help reveal the composition of planets outside of our solar system, but also could demonstrate evidence of water on those exoplanets.
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