Planetary Science News

New Research Provides More Evidence that Venus is Volcanically Active Today

Artist’s impression of a volcano erupting on Venus. Image credit: ESA / AOES Medialab.
Jan 6, 2020 by News Staff

Young lava flows detected by ESA’s Venus Express spacecraft are just few years old, according to new research from Universities Space Research Association (USRA). An artist’s impression of a volcano erupting on Venus. Image credit: ESA / AOES Medialab. In 2010, Venus Express scientists reported that the infrared radiation coming from three regions on Earth’s neighbor planet was different to that from the surrounding terrain. The researchers...

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Martian moon Phobos. Image credit: NASA / JPL-Caltech / University of Arizona.

Mars Express Captures New Views of Martian Moon Phobos

Dec 17, 2019 by News Staff

On November 17, 2019, ESA’s Mars Express orbiter made a close flyby of Phobos, the larger and inner of the two natural satellites of Mars. The probe...

A series of JunoCam images from Juno’s 23rd close science pass by Jupiter on November 3, 2019, revealed a sixth circumpolar cyclone in the cluster around Jupiter’s south pole. Image credit: NASA / JPL-Caltech / SwRI / MSSS.

Juno Spots New Circumpolar Cyclone at Jupiter’s South Pole

Dec 14, 2019 by News Staff

NASA’s Juno spacecraft spied the new Jovian cyclone on November 3, 2019, during its 23rd science pass of the gas giant. A series of JunoCam images from...

Computer-generated visualization of the orbital paths (white dots) taken by NASA’s MAVEN spacecraft as it mapped winds (blue lines) in the Martian upper atmosphere; red lines coming from the white dots represent local wind speed and direction, measured by MAVEN’s Neutral Gas and Ion Mass Spectrometer instrument. Image credit: NASA’s Goddard Space Flight Center / MAVEN / SVS / Greg Shirah.

NASA’s MAVEN Orbiter Maps Martian Upper Atmospheric Winds

Dec 13, 2019 by News Staff

Using NASA’s Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft, a team of planetary researchers have measured the speed and direction of winds...

On Earth, the Northern and Southern lights occur when the solar wind (electrically charged particles from the Sun) follow our planet’s geomagnetic field lines to the poles and collide with the upper atmosphere. Mars lacks a global magnetic field, so instead the solar wind piles up in front of Mars in a bow shock, which blocks charged particles from reaching the bulk of the atmosphere. However, in a process first observed by NASA’s MAVEN spacecraft, some solar wind protons can slip past the bow shock by first bonding with electrons from the Martian upper atmosphere to form hydrogen atoms. Because these hydrogen atoms are electrically neutral, they can pass through the bow shock and go on to create an ultraviolet proton aurora on the dayside of Mars. Image credit: NASA’s Goddard Space Flight Center.

‘Proton Aurora’ is Most Common Type of Aurora on Mars, Researchers Say

Dec 13, 2019 by News Staff

Proton aurora, a type of Martian aurora first identified in 2016, forms when protons from the solar wind interact with hydrogen in the extended portions...

This map shows near-surface water ice on Mars; cool colors represent less than one foot (30 cm) below the surface; warm colors are over two feet (60 cm) deep; sprawling brown zones on the map represent areas where a landing spacecraft would sink into fine dust; the outlined box represents the ideal region to send astronauts for them to be able to dig up water ice. Image credit: NASA / JPL-Caltech / ASU.

New Map Shows Near-Surface Water Ice on Mars

Dec 12, 2019 by News Staff

Using data from NASA’s Mars Reconnaissance Orbiter and Mars Odyssey orbiter, a team of planetary researchers have crated a map of the water ice depth...

Enceladus’ tiger stripes are known to be spewing ice from the moon’s icy interior into space, creating a cloud of fine ice particles over the moon’s south pole and creating Saturn’s mysterious E-ring. Evidence for this has come from NASA’s Cassini spacecraft that orbited Saturn from 2004 to 2017. Pictured here, a high resolution image of Enceladus is shown from a close flyby. Tiger stripes are visible in false-color blue. Image credit: NASA / ESA / JPL / SSI / Cassini Imaging Team.

Enceladus’ Tiger Stripes Finally Explained

Dec 10, 2019 by News Staff

Saturn’s 300-mile- (500 km) diameter moon Enceladus is thought to have an outer ice shell covering a liquid water ocean. Slashed across the moon’s...

The yellow-white cloud in the bottom-center of this image, taken on November 30, 2010 by NASA’s Mars Reconnaissance Orbiter, is a ‘dust tower’ -- a concentrated cloud of dust that can be lofted dozens of miles above the surface. The blue-white plumes are water vapor clouds. Image credit: NASA / JPL-Caltech / MSSS.

‘Dust Towers’ Spotted on Mars

Nov 28, 2019 by News Staff

NASA’s Mars Reconnaissance Orbiter observed a high number of ‘dust towers’ — concentrated clouds of dust that warm in sunlight and rise high...

This image shows a region of Mars named Deuteronilus Mensae. The oblique perspective view was generated using a digital terrain model and Mars Express data gathered on February 25, 2018. Image credit: ESA / DLR / FU Berlin / CC BY-SA 3.0 IGO.

ESA’s Mars Express Orbiter Spots Fractured Ice Sheets

Nov 26, 2019 by News Staff

The two Martian hemispheres are drastically different; the smooth northern lowlands sit up to 3 km below the rugged southern highlands, and the surface...

SEM image of the Acfer 094 polished section. CAI - Ca-Al-rich inclusion. Image credit: Matsumoto et al, doi: 10.1126/sciadv.aax5078.

Scientists Find Fossil Asteroidal Ice in Meteorite

Nov 26, 2019 by News Staff

An international team of scientists from the UK and Japan has found ‘fossilized asteroidal ice’ and pristine dust materials in a 4.6-billion-year-old...

Wing of Mars insect caught on the rover; inset: enlarged portion of wing. Image credit: William Romoser, doi: 10.13140/RG.2.2.12363.95520.

NASA Photos Show Insect- and Reptile-Like Life Forms on Mars, Entomologist Says

Nov 21, 2019 by News Staff

Ohio University Emeritus Professor William Romoser has analyzed photos from NASA’s various Mars rovers, mostly from the rover Curiosity, and found insect/arthropod-...

A model of the molecular structure of ribose and an image of the Murchison meteorite. Image credit: Yoshihiro Furukawa.

Researchers Find Extraterrestrial Sugars in Meteorites

Nov 20, 2019 by News Staff

An international team of scientists from Japan and the United States has found ribose and other bioessential sugars in two primitive meteorites, NWA 801...

The global geologic map of Titan. Image credit: NASA / JPL-Caltech / ASU.

Researchers Create Global Geologic Map of Saturn’s Moon Titan

Nov 19, 2019 by News Staff

Using radar and infrared data from NASA’s Cassini orbiter spacecraft, a team of planetary geologists has identified and mapped the major geological units...

This image from NASA’s Mars Reconnaissance Orbiter shows Jezero Crater on Mars, the landing site for NASA’s Mars 2020 mission. On ancient Mars, water carved channels and transported sediments to form fans and deltas within lake basins. Examination of spectral data acquired from orbit show that some of these sediments have minerals that indicate chemical alteration by water. Here in Jezero Crater delta, sediments contain clays and carbonates. Image credit: NASA / JPL-Caltech / MSSS / JHU-APL.

NASA’s Mars Reconnaissance Orbiter Finds Hydrated Silica in Jezero Crater

Nov 14, 2019 by News Staff

Using data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) instrument aboard NASA’s Mars Reconnaissance Orbiter, researchers have...

Curiosity rover took this selfie on October 11, 2019. The rover drilled twice in this location, nicknamed Glen Etive. Just left of the rover are the two drill holes, called Glen Etive 1 (right) and Glen Etive 2 (left). Image credit: NASA / JPL-Caltech / MSSS.

New Martian Mystery: Oxygen

Nov 12, 2019 by News Staff

The Sample Analysis at Mars (SAM) instrument onboard NASA’s Curiosity rover has measured the seasonal changes in the gases that fill the air directly...

Area of the study: (a) Valles Marineris, Mars, showing the location of the landslide in Coprates Chasma (white box); (b) stereo-derived DEMs; (c and d) study areas within which morphological and morphometric characterization is conducted; burgundy lines: topographic profiles, numbered from proximal to distal edge of the landslide deposit; blue lines: longitudinal ridges; (e) oblique view of the landslide object of the study; red lines represent topographic profiles, numbered from proximal to distal area (following flow direction). Image credit: Magnarini et al, doi: 10.1038/s41467-019-12734-0.

Planetary Researchers Analyze Structure of Giant Martian Landslide

Oct 25, 2019 by News Staff

Unusually large and long ridges documented in massive landslides across our Solar System are commonly associated with the presence of ancient ice layers....

Curiosity rover took this selfie on October 11, 2019. The rover drilled twice in this location, nicknamed Glen Etive. Just left of the rover are the two drill holes, called Glen Etive 1 (right) and Glen Etive 2 (left). Image credit: NASA / JPL-Caltech / MSSS.

Curiosity Rover Snaps New Selfie on Mars

Oct 25, 2019 by News Staff

NASA’s Mars rover Curiosity snapped a view of itself and its surroundings on October 11, 2019 (the 2,553rd Martian day, or Sol, of its mission). The...

The moons of our Solar System are brimming with unusual landscapes. However, sometimes they look a little more familiar, as in this new radar image from the Cassini orbiter. The image shows dark streaks carved into dunes reminiscent of those we might find on a beach on Earth, or raked with flowing lines in a Japanese Zen garden — but this scene is actually taking place on Saturn’s moon Titan. While our sand is composed of silicates, the ‘sand’ of these alien dunes is formed from grains of organic materials about the same size as particles of our beach sand. The small size and smoothness of these grains means that the flowing lines carved into the dunes show up as dark to the human eye. While previous images have spotted these eerily familiar patterns on Titan's dunes, this new image (colorized) shows them in greater detail. The image was obtained by Cassini's radar mapper on July 10, 2013. The vertical seam near the center is an artifact of radar image data processing. Image credit: NASA / JPL-Caltech / Sci-News.com.

Researchers Unravel Origin and Chemical Composition of Titan’s Mysterious Dunes

Oct 22, 2019 by News Staff

Vast longitudinal dunes up to 330 feet (100 m) in height in the equatorial deserts of Saturn’s moon Titan are the Solar System’s most monumental surface...

Venus in real colors, processed from Mariner 10 images. Image credit: Mattias Malmer / NASA.

Venus May Never Have Been Wet and Warm World

Oct 16, 2019 by News Staff

A team of planetary researchers from the Lunar and Planetary Institute (LPI) and elsewhere has found that a volcanic flow on Venus’ Ovda Regio highlands...

If the Moon has enough water

Lunar Water Ice May Have Multiple Sources, Researchers Say

Oct 11, 2019 by News Staff

Lunar orbiters such as India’s Chandrayaan-1 spacecraft and NASA’s Lunar Reconnaissance Orbiter (LRO) recently detected water icy on the floor of some...

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