Category Astronomy/Space

Deep Groundwater may Generate Surface Streams on Mars

Recurrent Slope Linae on the Palikir Crater walls on Mars.
Credit: NASA/JPL/University of Arizona

New research suggests that deep groundwater could still be active on Mars and could originate surface streams in some near-equatorial areas on Mars. In mid-2018, researchers supported by the Italian Space Agency detected the presence of a deep-water lake on Mars under its south polar ice caps. Now, researchers at the USC Arid Climate and Water Research Center (AWARE) have published a study that suggests deep groundwater could still be active on Mars and could originate surface streams in some near-equatorial areas on Mars.

The researchers at USC have determined that groundwater likely exists in a broader geographical area than just the poles of Mars and that there is an active system, as d...

Read More

Rivers Raged on Mars late into its history

A photo of a preserved river channel on Mars, taken by an orbiting satellite, with color overlaid to show different elevations (blue is low, yellow is high).
Credit: NASA/JPL/Univ. Arizona/UChicago

This complicates the picture for scientists trying to model the ancient Martian climate, said lead study author Edwin Kite, assistant professor of geophysical sciences and an expert in both the history of Mars and climates of other worlds. “It’s already hard to explain rivers or lakes based on the information we have,” he said. “This makes a difficult problem even more difficult.”

But, he said, the constraints could be useful in winnowing the many theories researchers have proposed to explain the climate.

Mars is crisscrossed with the distinctive tracks of long-dead rivers...

Read More

In Hunt for Life, Astronomers Identify most Promising Stars


Artists’ concept of the Transiting Exoplanet Survey Satellite against a background of stars and orbiting planets in the Milky Way.
Credit: European Space Agency, European Southern Observatory and NASA’s Goddard Space Flight Center

NASA’s new Transiting Exoplanet Survey Satellite (TESS) is designed to ferret out habitable exoplanets, but with hundreds of thousands of sunlike and smaller stars in its camera views, which of those stars could host planets like our own?

TESS will observe 400,000 stars across the whole sky to catch a glimpse of a planet transiting across the face of its star, one of the primary methods by which exoplanets are identified.

A team of astronomers from Cornell University, Lehigh University and Vanderbilt University has identified the most promising targe...

Read More

Icy Giant Planets in the Laboratory

Even under extremely high pressure, such as those in the interior of Neptune or Uranus, there are stable crystal structures of carbon (orange) and hydrogen (gray). This discovery by HZDR researchers reveals new possibilities for the inner structure of the ice giants.
Credit: HZDR / J. Vorberger

Researchers use plastics to better understand what happens inside planets. Giant planets like Uranus and Neptune may contain much less free hydrogen than previously assumed. Researchers from the German Helmholtz-Zentrum Dresden-Rossendorf (HZDR) drove shock waves through two different types of plastic to reach the same temperatures and pressures present inside such planets, and observed the behavior using ultra-strong X-ray laser pulses...

Read More