Planetary Science News

If the Moon has enough water, and if it’s reasonably convenient to access, future explorers might be able to use it as drinking water or to convert it into hydrogen and oxygen for rocket fuel or oxygen to breathe. Image credit: NASA’s Goddard Space Flight Center.

Water is Widely Distributed across Lunar Surface, Study Suggests

Feb 26, 2018 by News Staff

A new study published in the journal Nature Geoscience indicates that water may be more prevalent on the lunar surface than previously thought. If the...

Mars is kept company by two cratered moons -- an inner moon named Phobos and an outer moon named Deimos. Image credit: NASA / JPL-Caltech / Malin Space Science Systems / Texas A&M University.

Tiny Martian Moons Hint at Red Planet’s Adolescent Rejection

Feb 13, 2018 by James Romero

Like a teenage diary you can’t throw away, Mars might carry a reminder of its difficult formative years in its tiny moons. A paper published by the Royal...

Two 2001 images from the Mars Orbiter Camera on NASA’s Mars Global Surveyor show a dramatic change in the planet’s appearance when haze raised by dust-storm activity in the south became globally distributed. The images were taken about a month apart. Image credit: NASA / JPL-Caltech / MSSS.

Martian Dust Storms Linked to Atmospheric Gas Escape

Jan 25, 2018 by News Staff

Martian dust storms play a role in the ongoing process of gas escaping from the top of the planet’s atmosphere, according to a new study using observations...

Top: stereographic polar projections of Titan’s topography with the South Pole left and the North Pole right; Ontario Lacus and the each of the large northern seas are found in local depressions. Bottom: equicylindrical projection of Titan’s topography. All maps have been corrected for the geoid. Image credit: Corlies et al, doi: 10.1002/2017GL075518.

Planetary Researchers Create New Global Topographic Map of Saturn’s Moon Titan

Jan 19, 2018 by News Staff

Using data from NASA’s Cassini spacecraft, a team of planetary researchers led by Cornell University has produced a new global topographic map of Titan,...

Gale Crater is 96 miles (154 km) in diameter and holds a layered mountain rising about 3 miles (5 km) above the crater floor. Image credit: NASA / JPL-Caltech / ASU / UA.

Mars’ Turbulent Winds Can Make Mountains in Impact Craters

Jan 15, 2018 by News Staff

In a paper published in the journal Physical Review E, a duo of fluid dynamics experts proposes a solution to one of long-standing Martian mysteries. The...

This high-resolution HiRISE image shows a detailed subsection of an icy scarp on Mars in enhanced color. Image credit: NASA / JPL / University of Arizona / USGS.

New HiRISE Images Show 3D Structure of Martian Ice Sheets

Jan 12, 2018 by News Staff

New images from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter reveal never-before-observed details...

A salt crystal recovered from the Zag meteorite. Image credit: Queenie Chan, Open University.

Scientists Find Primordial Organic Matter in Two Meteorites

Jan 11, 2018 by News Staff

A team of researchers from the United States, UK and Japan has found liquid water and a mix of complex organic compounds in 4.5-billion-year-old salt crystals...

This image shows how the solar wind transports ions of oxygen from the Earth’s atmosphere to the Moon. Image credit: Osaka University / NASA.

Moon Has Earth’s Oxygen, Planetary Researchers Say

Jan 2, 2018 by News Staff

A team of Japanese planetary researchers led by Osaka University’s Professor Kentaro Terada has discovered that the solar wind and Earth’s magnetic...

Saturn’s Great Northern Storm churning through the atmosphere in the planet’s northern hemisphere overtakes itself as it encircles the planet in this true-color view from NASA’s Cassini spacecraft. This picture, captured on February 25, 2011, was taken about 12 weeks after the storm began, and the clouds by this time had formed a tail that wrapped around the gas giant. Image credit: NASA / JPL-Caltech / Space Science Institute.

Saturn’s Northern Storms Cause Disturbances in Its ‘Heartbeat’

Dec 31, 2017 by News Staff

Giant storms in Saturn’s northern hemisphere can disturb atmospheric patterns at the ringed giant’s equator, according to new research published in...

This artist’s concept depicts the dry environment seen at Mars today versus the early Martian environment. Image credit: Simon Fraser University.

Study: Martian Surface Water Was Absorbed by Planet’s Crust

Dec 24, 2017 by News Staff

According to a new study published in the journal Nature, the Sun may not have evaporated away all of the Martian surface water after all; instead, Mars’...

A 1.5-mm-long impact track of a meteoroid captured in aerogel exposed to space by the European Retrievable Carrier (EURECA) spacecraft. Image credit: NASA / ESA.

Simulations Reveal Why Meteoroids Explode Before They Reach Earth

Dec 13, 2017 by News Staff

According to a paper published in the journal Meteoritics & Planetary Science, Earth’s atmosphere is a better shield from meteoroids than scientists...

This full-disc image of Jupiter was taken on 21 April 2014 with Hubble's Wide Field Camera 3. Image credit: NASA / ESA / A. Simon, Goddard Space Flight Center.

NASA’s Juno Orbiter Explores Depths of Jupiter’s Great Red Spot

Dec 12, 2017 by News Staff

Data collected by Juno during its first pass over Jupiter’s mysterious, roiling storm called the Great Red Spot in July 2017 indicate that this famous...

Mars may have been enveloped in a steamy atmosphere as the planet’s crust cooled and solidified. That ‘steam bath’ could have created many of the clay mineral deposits that have long been attributed to water flow on or just beneath the Martian surface. Image credit: Kevin Cannon.

Research Suggests Martian Clays Formed in Ancient ‘Steam Bath’

Dec 7, 2017 by News Staff

On Mars, phyllosilicate (clay) minerals are widespread in terrains that date back to the Noachian period, 4.1 to 3.7 billion years ago. Phyllosilicates...

Marchi et al modeled the protracted period of bombardment after the Moon formed, determining that impactor metals may have descended into Earth’s core. This artistic rendering illustrates a large impactor crashing into the young Earth. Light brown and gray particles indicate the projectile’s mantle (silicate) and core (metal) material, respectively. Image credit: Southwest Research Institute.

Large Planetesimals Delivered More Mass to Proto-Earth than Previously Thought

Dec 5, 2017 by News Staff

After the Moon’s formation, Earth experienced a protracted bombardment by large (over 1,500 km in diameter) planetesimals. Dr. Simone Marchi, a researcher...

The surface of Europa looms large in this newly-reprocessed color view; image scale is 1.6 km per pixel; north on Europa is at right. Image credit: NASA / JPL-Caltech / SETI Institute.

Research Provides New Evidence of Plate Tectonics in Europa’s Ice Shell

Dec 5, 2017 by News Staff

A process called subduction — when a tectonic plate slides underneath another and sinks deep into a planetary body’s interior — is physically...

Titan’s south polar vortex stands out against the orange and blue haze layers that are characteristic of the hazy moon’s atmosphere. This view looks towards the trailing hemisphere of Titan (3,200 miles, or 5,150 km across). North on Titan is up and rotated 17 degrees to the left. Images taken using red, green and blue spectral filters were combined to create this natural-color view. The image was taken with the Cassini spacecraft narrow-angle camera on July 30, 2013. The view was acquired at a distance of approximately 895,000 miles (1.441 million km) from Titan. Image credit: NASA / JPL-Caltech / Space Science Institute.

New Study Explains Unexpected Cooling of Titan’s Polar Atmosphere

Nov 24, 2017 by News Staff

A study published in the journal Nature Communications has shown that a recently reported unexpected polar vortex behavior on Saturn’s hazy moon Titan...

According to Zhang et al, Pluto’s atmosphere is unique among Solar System planetary atmospheres, as its equilibrium temperature is controlled primarily by solid-phase haze particles instead of gas molecules. This artist’s impression shows a view of the moon Charon through Pluto’s atmospheric haze layers above the mountain landscape of bedrock water ice covered partially with deposition of dark, reddish haze particles. Image credit: X. Liu.

Haze Particles Cool Pluto’s Atmosphere, New Research Finds

Nov 21, 2017 by News Staff

It turns out solid-phase haze particles help cool the atmosphere of the dwarf planet Pluto. That’s according to new research by planetary scientists...

$This false-color image demonstrates how use of special filters available on Curiosity’s Mastcam camera can reveal the presence of certain minerals in target rocks. It is a composite of images taken through three ‘science’ filters chosen for making hematite stand out as exaggerated purple. Mastcam’s narrow-band filters used for this view help to increase spectral contrast, making blues bluer and reds redder, particularly with the processing used to boost contrast in each of the component images of this composite. Fine-grained hematite preferentially absorbs sunlight around in the green portion of the spectrum around 527 nm. That gives it the purple look from a combination of red and blue light reflected by the hematite and reaching the camera through the other two filters. Bright lines within the rocks are fractures filled with calcium sulfate minerals. Image credit: NASA / JPL-Caltech / MSSS.$

NASA’s Curiosity Rover Finds Mineral Hematite on Mars

Nov 12, 2017 by News Staff

NASA’s Curiosity rover has found spectral evidence of an iron-oxide mineral called hematite (Fe2O3) on a rock near Mount Sharp in Gale Crater, Mars. This...

This graphic illustrates how water might be heated inside Enceladus. Over time, cool ocean water seeps into the moon’s porous core. Pockets of water reaching deep into the interior are warmed by contact with rock in the tidally heated interior and subsequently rise owing to the positive buoyancy, leading to further interaction with the rocks. The heat deposited at the boundary between the seafloor and ocean powers hydrothermal vents. Heat and rocky particles are transported through the ocean, triggering localized melting in the icy shell above. This leads to the formation of fissures, from which jets of water vapor and the rocky particles from the seafloor are ejected into space. In the graphic, the interior ‘slice’ is an excerpt from a new model that simulated this process. The orange glow represents the parts of the core where temperatures reach at least 194 degrees Fahrenheit. Tidal heating owing to the friction arising between particles in the porous core provides a key source of energy, but is not illustrated in this graphic. The tidal heating results primarily from the gravitational pull from Saturn. Image credit: NASA / JPL-Caltech / Space Science Institute / LPG-CNRS / University of Nantes / University of Angers / ESA.

Enceladus’ Highly Porous Core Keeps Its Subsurface Ocean Warm, New Study Says

Nov 8, 2017 by News Staff

A new modeling study led by the University of Nantes is the first to explain several key characteristics of Saturn’s moon Enceladus observed by NASA’s...