3 Questions: Evidence for planetary formation through gravitational instability
Assistant Professor Richard Teague describes how movement of unstable gas in a protoplanetary disk lends credibility to a secondary theory of planetary formation.
Assistant Professor Richard Teague describes how movement of unstable gas in a protoplanetary disk lends credibility to a secondary theory of planetary formation.
The presence of organic matter is inconclusive, but the rocks could be scientists’ best chance at finding remnants of ancient Martian life.
The barely-there lunar atmosphere is likely the product of meteorite impacts over billions of years, a new study finds.
The planet’s wild orbit offers clues to how such large, hot planets take shape.
New findings challenge current thinking on the ocean’s role in storing carbon.
MIT researchers find wave activity on Saturn’s largest moon may be strong enough to erode the coastlines of lakes and seas.
Circling a cold, Jupiter-sized star, the new world could offer an unobstructed view of its surface composition and history.
The new world is the second-lightest planet discovered to date.
The results suggest that climate may influence seismic activity.
The 3.7 billion-year-old rocks may extend the magnetic field’s age by 200 million years.
The new approach “nudges” existing climate simulations closer to future reality.
Results suggest the clouds of Venus could be hospitable for some forms of life.
With Project MADMEN, two MIT students experience the challenges and bonding associated with a Mars analog mission.
The “oriented” samples, the first of their kind from any planet, could shed light on Mars’ ancient magnetic field.
A low carbon abundance in planetary atmospheres, which the James Webb Space Telescope can detect, could be a signature of habitability.