Space Exploration News

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

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.
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 of the Martian atmosphere and travel to lower regions. According to multi-year observations made using the Imaging UltraViolet Spectrograph (IUVS) onboard NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) spacecraft, this phenomenon is actually the most common form of aurora on Mars; it is observed...

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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...

Schematic diagram of orbit determination model output for the 19 January 2019 particle ejection event from Bennu observed by the OSIRIS-REx spacecraft: Bennu is depicted in gray and has a diameter of 1,640 feet (500 m). OSIRIS-REx is indicated with the brown dot, 1.2 miles (2 km) from Bennu’s center of mass; the cone represents the viewing angle; blue arcs are particle trajectories, ending or with gaps where the trajectories pass into shadow; the Sun-angular momentum frame coordinates are shown at bottom right: x - solar vector, y - Bennu orbital direction, z - Bennu north. Image credit: Lauretta et al, doi: 10.1126/science.aay3544.

Bennu is Active Asteroid, OSIRIS-REx Team Says

Dec 11, 2019 by News Staff

NASA’s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) spacecraft recently observed several particle...

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...

Illustration of NASA’s Parker Solar Probe approaching the Sun. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Steve Gribben.

NASA Releases First Science Results from Parker Solar Probe Mission

Dec 6, 2019 by NASA

The four instruments of NASA’s Parker Solar Probe, a robotic spacecraft designed to explore the Sun’s atmosphere, have returned unprecedented science...

This schematic of the heliosphere shows the solar wind begins slowing at approximately 4 AU radial distance from the Sun and continues to slow as it moves toward the outer Solar System and picks up interstellar material. Current extrapolations reveal the termination shock may currently be closer than found by the Voyager spacecraft. However, increasing solar activity will soon expand the heliosphere and push the termination shock farther out, possibly to the 84-94 AU range encountered by the Voyager spacecraft. Image credit: Southwest Research Institute / NASA / Adler Planetarium.

Solar Wind Slows in Outer Heliosphere, Data from New Horizons Confirm

Dec 4, 2019 by News Staff

As the solar wind — the supersonic stream of charged particles blown out by the Sun — moves farther from the Sun, it encounters an increasing...

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...

The Expedition 20 crew members share a meal in the Unity node of the International Space Station. Image credit: NASA.

Spaceflight Can Cause Sustained Defect in Epithelial Barrier Function, New Study Shows

Nov 27, 2019 by News Staff

Epithelial cells that line our intestines serve as a robust barrier to invasion by viruses, bacteria and exposure to ingested agents. A new study, published...

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...

This composite image of Ultima Thule was compiled from data obtained by NASA’s New Horizons spacecraft as it flew by the object on January 1, 2019. The image combines enhanced color data (close to what the human eye would see) with detailed high-resolution panchromatic pictures. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute / Roman Tkachenko.

Kuiper Belt Object Ultima Thule Has New Name: Arrokoth

Nov 13, 2019 by News Staff

Ultima Thule (also known as 2014 MU69), the Kuiper Belt Object that was the target of the January 1, 2019 flyby by NASA’s New Horizons mission, has been...

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...

NASA’s Voyager 2 Spacecraft Sends Back New Data on Interstellar Space

Nov 5, 2019 by News Staff

In November 2018, NASA’s Voyager 2 spacecraft became only the second human-made object to cross the outer edge of the Sun’s heliosphere, the bubble...

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...

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