Planetary Science News

Dawn data show a region around Ceres’ Ernutet crater where organic concentrations have been discovered; the color coding shows the surface concentration of organics, as inferred from the visible and near infrared spectrometer; the inset shows a higher resolution enhanced color image of the crater acquired by Dawn’s framing camera; regions in red indicate higher concentration of organics. Image credit: NASA / JPL-Caltech / UCLA / ASI / INAF / MPS / DLR / IDA.

New Research Reveals Origin of Ceres’ Organic Matter

Oct 23, 2017 by News Staff

Organic-rich materials found on Ceres by NASA’s Dawn orbiter are native to the dwarf planet, according to new research led by Southwest Research Institute...

Volcanic activity 3.5 billion years ago released 1019 g of volatiles around the Moon. Image credit: NASA.

Moon Once Had Atmosphere, New Research Says

Oct 20, 2017 by News Staff

About 3.5 billion years ago volcanic activity on Earth’s only permanent natural satellite produced an atmosphere 1.5 times thicker than is currently...

Artist’s conception of the complex magnetic field environment at Mars. Yellow lines represent magnetic field lines from the Sun carried by the solar wind, blue lines represent Martian surface magnetic fields, white sparks are reconnection activity, and red lines are reconnected magnetic fields that link the surface to space via the Martian magnetotail. Image credit: Anil Rao / University of Colorado / MAVEN / NASA’s Goddard Space Flight Center.

Mars Has a Twisted Magnetotail, NASA Research Reveals

Oct 20, 2017 by News Staff

According to new research using data from NASA’s Mars Atmosphere and Volatile Evolution Mission (MAVEN) spacecraft, the Red Planet has an invisible magnetic...

This view of Titan is among the last images NASA’s Cassini spacecraft sent to Earth before it plunged into the giant planet’s atmosphere. Image credit: NASA / JPL-Caltech / Space Science Institute.

Toxic Ice Cloud Found in Titan’s Stratosphere

Oct 19, 2017 by News Staff

Planetary researchers with NASA’s Cassini mission have detected a cloud of toxic hybrid ice high above the south pole of Saturn’s hazy moon, Titan. This...

Powerful Solar Storms Could Electrically Charge Mars’ Moon Phobos

Oct 18, 2017 by News Staff

A new study published in the journal Advances in Space Research suggests that solar storms create a complex electrical environment around Phobos, giving...

It’s raining on Titan. Image credit: David A. Hardy, AstroArt / NASA.

Heavy Methane Rainstorms Batter Titan, Researchers Say

Oct 13, 2017 by News Staff

Saturn’s hazy moon has surprisingly extreme rainstorms, according to new research published in the journal Nature Geoscience. It’s raining on Titan....

Mars’ Eridania Basin Once Held Vast Sea

Oct 9, 2017 by News Staff

NASA’s Mars Reconnaissance Orbiter (MRO) has identified what appear to be ancient hydrothermal deposits in the Eridania region in the southern highlands...

Mars Odyssey spotted possible water ice in the Medusa Fossae area of Mars, which is in an equatorial region of the planet to the lower left in this view. Image credit: Steve Lee, University of Colorado / Jim Bell, Cornell University / Mike Wolff, Space Science Institute / NASA.

NASA’s Mars Odyssey Orbiter Spots Possible Water Ice near Martian Equator

Oct 2, 2017 by News Staff

NASA’s Mars Odyssey spacecraft has discovered evidence of significant hydration near the Martian equator. Mars Odyssey spotted possible water ice in...

Pluto’s bladed terrain as seen from NASA’s New Horizons spacecraft during its July 2015 flyby. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute.

Planetary Researchers Solve Mystery of Pluto’s ‘Bladed Terrain’

Sep 27, 2017 by News Staff

Strange formations are found at the highest altitudes on the surface of the dwarf planet Pluto. They resemble giant knife blades of ice and can soar many...

A young planetary system. Image credit: NASA / FUSE / Lynette Cook.

Research Sheds Light on Sequence of Events that Led to Creation of Earth and Mars

Sep 27, 2017 by News Staff

New research, reported in the journal Nature, changes scientists’ understanding of how terrestrial planets attain their physical and chemical characteristics. A...

Large, smooth areas on Vesta correlated with higher concentrations of hydrogen. Image credit: Elizabeth Palmer / Essam Heggy.

Dawn Data Provide New Evidence for Ground Ice on Asteroid Vesta

Sep 22, 2017 by News Staff

Using data from NASA’s Dawn spacecraft, researchers have found new evidence for the occurrence of ground ice on Vesta, the second largest asteroid of...

Deutsch et al found new evidence of ice sheets in permanently shadowed craters near the north pole of the planet Mercury. Image credit: Brown University.

Scientists Find New Evidence for Surface Water Ice at Mercury’s North Pole

Sep 21, 2017 by News Staff

A new study led by Brown University planetary researchers adds three new large members to the list of water ice-filled craters near Mercury’s north pole...

Aeolis Dorsa, Mars: the dotted white arrow points to curved strata recording point bar growth and river migration; the boundaries of ancient valley walls are defined by textural and albedo changes and are also associated with lateral river migration; stacked above the point bars and completely confined within the dotted white and black lines are topographically inverted river deposits outcropping as ridges (e.g., black arrow); in places (e.g., south of the dotted white arrow), the ridges run against the dotted boundaries, suggesting flow was once redirected along a valley wall. Image credit: Cardenas et al, doi: 10.1130/B31567.1.

Planetary Researchers Find More Evidence of Water on Early Mars

Sep 19, 2017 by Enrico de Lazaro

River deposits exist across the Martian surface. A large sedimentary basin named Aeolis Dorsa contains some of the planet’s most spectacular and densely...

A new map of the thickness of the Martian crust shows less variation between thicker regions (red) and thinner regions (blue), compared to earlier mapping. This view is centered on Valles Marineris, with the Tharsis Montes near the terminator to its west. The map is based on modeling of Mars’ gravity field by Goossens et al. Image credit: NASA / Goddard / UMBC / MIT / E. Mazarico.

Martian Crust is Relatively Porous, Planetary Scientists Find

Sep 15, 2017 by News Staff

A team of researchers led by Dr. Sander Goossens of NASA’s Goddard Space Flight Center has found evidence that the crust of the Red Planet is not as...

This image, created with data from Juno’s Ultraviolet Imaging Spectrograph, marks the path of Juno’s readings of Jupiter’s auroras, highlighting the electron measurements that show the discovery of discrete auroral acceleration processes indicated by the ‘inverted Vs’ in the lower panel. Image credit: NASA / JPL-Caltech / SwRI / Randy Gladstone.

Juno Detects Vast Amounts of Energy over Jupiter’s Auroral Regions

Sep 11, 2017 by News Staff

In a paper published in the journal Nature, Dr. Barry Mauk of the Johns Hopkins University Applied Physics Laboratory and co-authors report observations...

An illustration of JAXA’s Akatsuki orbiter successfully tracking lower-altitude clouds during the night with its near-infrared camera IR2. Image credit: PLANET-C Project Team.

JAXA’s Akatsuki Orbiter Spots Equatorial Jet in Venus’ Atmosphere

Sep 1, 2017 by News Staff

New observations from Akatsuki, a robotic spacecraft launched by the Japan Aerospace Exploration Agency (JAXA) in 2010 to orbit Venus, have revealed an...

Oxo Crater is the second-brightest feature on Ceres. Only Occator’s central area is brighter. Oxo lies near the 0 degree meridian that defines the edge of many Ceres maps, making this small feature easy to overlook. NASA’s Dawn spacecraft took this image in its low-altitude mapping orbit, at a distance of 385 km from the surface of Ceres. Image credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA / PSI.

Crater Slope Avalanches Reveal Ceres’ Surface Water Ice

Aug 25, 2017 by James Romero

Surface water ice found within a brilliantly bright crater on the dwarf planet Ceres is being exposed by avalanches reprocessing impact deposits in just...

Moon’s Interior Likely Contains No Water, New Research Says

Aug 22, 2017 by News Staff

A new study led by a Scripps Institution of Oceanography researcher contradicts a recently published paper, which suggested the interior of Earth’s only...

A cutaway depicts the interior of Neptune (left). In the new experiment, Kraus et al studied a plastic simulating compounds formed from methane -- a molecule with just one carbon bound to four hydrogen atoms that causes the distinct blue cast of Neptune; methane forms hydrocarbon (hydrogen and carbon) chains that respond to high pressure and temperature to form ‘diamond rain’ in the interiors of ice giants like Neptune; the authors were able to recreate similar conditions using high-powered optical lasers and watch the small diamonds form in real time with X-rays. Image credit: Greg Stewart, SLAC National Accelerator Laboratory.

It Rains Diamonds on ‘Ice Giant’ Planets

Aug 21, 2017 by News Staff

A new experiment at SLAC National Accelerator Laboratory reveals how large diamonds may be formed from just hydrogen and carbon in the deep interior of...