Planetary Science News

Molecular hydrogen points to hydrothermal activity in an ocean beneath the icy surface of Enceladus. Image credit: NASA / JPL-Caltech.

Cassini Finds New Evidence for Hydrothermal Processes in Enceladus’ Ice-Covered Ocean

Apr 13, 2017 by News Staff

During NASA’s Cassini spacecraft’s deepest-ever dive through Enceladus’ plume of gas and ice grains, researchers discovered molecular hydrogen in...

MAVEN is exploring Mars’ upper atmosphere in detail to understand how Mars changed from a wet planet early in its history to the cold, dry world we see today. Image credit: NASA’s Goddard Space Flight Center.

MAVEN Detects Metal Ions in Martian Atmosphere

Apr 11, 2017 by News Staff

NASA’s Mars Atmosphere and Volatile EvolutioN (MAVEN) mission has made the first detection of the continuous presence of iron, magnesium, and sodium...

Occator crater on Ceres. Image credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA.

Ceres’ Transient Exosphere is Product of Solar Activity, Planetary Researchers Say

Apr 10, 2017 by News Staff

Planetary researchers have long thought that the dwarf planet Ceres may have a temporary, thin atmosphere (an exosphere), but mysteries lingered about...

This image shows ancient Mars capable of supporting liquid water on its surface. Image credit: Michael Lentz / NASA Goddard Conceptual Image Lab.

MAVEN Finds New Evidence that Most of Martian Atmosphere Was Lost to Space

Mar 31, 2017 by News Staff

According to an analysis of new data from NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) spacecraft, solar wind and radiation are responsible...

An artist’s rendering of the surface of Saturn’s largest moon, Titan. Image credit: Benjamin de Bivort, debivort.org / CC BY-SA 3.0.

Titan Has ‘Electrically-Charged’ Hydrocarbon Sands

Mar 29, 2017 by News Staff

Low-density organic granules that cover the surface of Saturn’s moon Titan are ‘electrically charged,’ according to new experiments done by scientists...

This digital-image mosaic of Mars’ Tharsis plateau shows the extinct volcano Arsia Mons. It was assembled from images that NASA’s Viking 1 orbiter took during its 1976-1980 working life at Mars. Image credit: NASA / JPL / USGS.

Martian Shield Volcano Arsia Mons Was Last Active 50 Million Years Ago, Research Reveals

Mar 21, 2017 by News Staff

According to new research reported in the journal Earth and Planetary Science Letters, the 10-mile- (16 km) high Martian shield volcano called Arsia Mons...

Every discovered planet in the Solar System under 10,000 km in diameter, to scale. The geophysical definition of planet includes 110 known planets. Image credit: Emily Lakdawalla, Planetary Society / K.D. Runyon et al.

Planet Count May Reach 110

Mar 21, 2017 by Enrico de Lazaro

Kirby Runyon, a PhD candidate in planetary geology at the Johns Hopkins University, and co-authors are proposing to rewrite the textbooks to say that the...

$This enhanced-color view of Enceladus is largely of the southern hemisphere and includes the south polar terrain at the bottom of the image. Ancient craters remain somewhat pristine in some locales, but have clearly relaxed in others. Northward-trending fractures, likely caused by a change in the moon’s rate of rotation and the consequent flattening of the moon’s shape, rip across the southern hemisphere. The south polar terrain is marked by a striking set of ‘blue’ fractures and encircled by a conspicuous and continuous chain of folds and ridges, testament to the forces within Enceladus that have yet to be silenced. The mosaic was created from 21 false-color frames taken during Cassini’s close approaches to Enceladus on March 9 and July 14, 2005. Images taken using filters sensitive to UV, visible and IR light (spanning wavelengths from 338 to 930 nm) were combined to create the individual frames. Image credit: NASA / JPL / Space Science Institute.$

Cassini Spots Anomalously Warm Subsurface Region on Enceladus

Mar 16, 2017 by News Staff

A new study, based on microwave observations by NASA’s Cassini orbiter, shows that the south polar region of Saturn’s frozen moon Enceladus is warmer...

Cerealia Facula, a bright dome in the center of Occator Crater on the dwarf planet Ceres, is shown in enhanced color in this view from NASA’s Dawn spacecraft. Image credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA / PSI / LPI.

Researchers Determine Age of Ceres’ Brightest Spot

Mar 10, 2017 by News Staff

Cerealia Facula, a dome-like feature located in the center of Ceres’ Occator crater, is only 4 million years old — approximately 30 million years...

Blue skies on Pluto. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute.

The Secrets of Pluto’s Thin Blue Line

Mar 3, 2017 by James Romero

“Like a summer’s evening here on Earth just after sunset. A faint blue glow follows the Sun below the horizon — the only bit of color within...

This is a three-color composite image of Saturn and its rings taken January 23, 2008 with the COMICS instrument on the Subaru Telescope. The Cassini Division and the C ring appear bright. Color differences reflect the temperatures; the warmer part is blue, the cooler part is red. Image credit: NAOJ.

Researchers Measure Brightness, Temperatures of Saturn’s Main Rings

Mar 2, 2017 by Enrico de Lazaro

Using mid-infrared data from the 8.2-m Subaru Telescope, a research team led by Dr. Hideaki Fujiwara, Subaru scientist at the National Astronomical Observatory...

A large pit valley in Lucaya crater, Mars: (a) exposure of putative crossbeds on windward slope of dunes, and (b) interdune strata exposed in planform showing contrasting albedo and crosscutting relationships similar to that exposed in the dune. Image credit: M.C. Bourke & H.A. Viles.

Researchers Uncover New Evidence for Water on Ancient Mars

Feb 19, 2017 by News Staff

Dr. Mary Bourke from Trinity College Dublin and University of Oxford Professor Heather Viles have discovered a patch of land in an equatorial crater on...

This enhanced color composite image, made with data from NASA’s Dawn spacecraft, shows the area around Ernutet crater, which is about 32 miles (52 km) in diameter and is located in the northern hemisphere. The bright red portions appear redder with respect to the rest of Ceres. In the new study, planetary researchers found that these red areas around Ernutet are associated with evidence of organic material. Images taken using blue (440 nm), green (750 nm) and infrared (960 nm) spectral filters were combined to create the view. Image credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA.

Aliphatic Organic Compounds Detected on Ceres

Feb 17, 2017 by News Staff

An international team of planetary researchers has discovered the presence of aliphatic organic compounds — carbon-based building blocks that may...

This artist’s rendering illustrates a conceptual design for a potential future mission to land a robotic probe on the surface of Europa. The lander is shown with a sampling arm extended, having previously excavated a small area on the surface. The circular dish on top is a dual-purpose high-gain antenna and camera mast, with stereo imaging cameras mounted on the back of the antenna. Three vertical shapes located around the top center of the lander are attachment points for cables that would lower the rover from a sky crane, which is envisioned as the landing system for this mission concept. Image credit: NASA / JPL-Caltech / M. Carroll.

Science Report on NASA’s Europa Lander Concept Released

Feb 10, 2017 by News Staff

In a new report to NASA released this week, a 21-member team of scientists assess the scientific value and engineering design of a future mission to the...

This artist’s concept depicts the early Martian environment (right) -- believed to contain liquid water and a thicker atmosphere -- versus the cold, dry environment seen at Mars today (left). Image credit: NASA’s Goddard Space Flight Center.

Did Ancient Martian Volcanism Provide the Sunblock to Get Life Going?

Feb 8, 2017 by James Romero

Intense volcanism early in Mars history could have aided the emergence of life on the red planet through filtering out harmful ultraviolet (UV) radiation...

Ahuna Mons, Ceres’ lonely mountain, is seen in this simulated perspective view. The elevation has been exaggerated by a factor of two. The view was made using enhanced-color images from NASA’s Dawn orbiter. Images taken using blue (440 nm), green (750 nm) and infrared (960 nm) spectral filters were combined to create the view. The spacecraft’s framing camera took the images from Dawn’s low-altitude mapping orbit, from an altitude of 240 miles (385 km) in August 2016. Image credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA / PSI.

Ceres May Have Vanishing Cryovolcanoes

Feb 3, 2017 by News Staff

Ahuna Mons, a 2.5-mile- (4 km) tall mountain on Ceres interpreted as a geologically young cryovolcano, may have some hidden older siblings, according to...

Hand sample images of the cut NWA 7635 stone and a representative backscattered electron image of the igneous texture of the stone. Image credit: Thomas J. Lapen et al, doi: 10.1126/sciadv.1600922.

Rare Martian Meteorite Provides Clues to Red Planet’s Evolution

Feb 2, 2017 by News Staff

Northwest Africa (NWA) 7635 — a Martian meteorite found in Algeria in 2012 — has given planetary researchers information about volcanic activity...

This is an artist’s rendering of the space collision 466 million years ago that gave rise to many of the meteorites falling today. Image credit: Don Davis, Southwest Research Institute.

Study: Today’s Rare Meteorites Were Common in Ordovician Period

Jan 25, 2017 by News Staff

A new study published in the journal Nature Astronomy is the first to look at meteorites from before giant space collision 466 million years ago. This...

Mosaic of the Valles Marineris hemisphere of Mars projected into point perspective, a view similar to that which one would see from a spacecraft. The distance is 1,550 miles (2,500 km) from the surface of the planet. The mosaic is composed of 102 Viking Orbiter images of Mars. The center of the scene shows the entire Valles Marineris canyon system, over 1,240 miles (2,000 km) long and up to 5 miles (8 km) deep, extending form Noctis Labyrinthus, the arcuate system of graben to the west, to the chaotic terrain to the east. Many huge ancient river channels begin from the chaotic terrain from north-central canyons and run north. The three Tharsis volcanoes (dark red spots), each about 15.5 miles (25 km) high, are visible to the west. South of Valles Marineris is very ancient terrain covered by many impact craters. Image credit: NASA / JPL-Caltech.

Methane Gas May Have Caused Greenhouse Effect on Young Mars, Planetary Researchers Say

Jan 25, 2017 by News Staff

Methane present in the early Martian atmosphere, together with carbon dioxide and hydrogen may have created a greenhouse effect on the planet 3.5-4.5 billion...