Tag Archive for 'Planet'

This artist’s impression shows Proxima b orbiting Proxima Centauri, which at only 4.23 light-years is the closest star to our Solar System. The double star Alpha Centauri AB also appears in the image between the exoplanet and Proxima itself. Image credit: M. Kornmesser / ESO.

New Study Questions Exoplanet Proxima b’s Ability to Retain Earth-Like Atmosphere

Aug 2, 2017 by News Staff

According to new research from NASA scientists, Proxima b may not be able to keep a grip on its atmosphere, leaving the surface exposed to harmful radiation. This...

The atmospheric superrotation at the upper clouds of Venus. While the superrotation is present in both day and night sides of Venus, it seems more uniform in the day (AKATSUKI-UVI image, right), while in the night this seems to become more irregular and unpredictable (composite of Venus Express/VIRTIS images, left). Image credit: JAXA / ESA / J. Peralta, JAXA / R. Hueso, UPV/EHU.

Research Sheds New Light on Venus’ Superrotating Atmosphere

Jul 28, 2017 by Enrico de Lazaro

A team of researchers led by JAXA’s Institute of Space and Astronautical Science has discovered unexpected patterns of slow motion and stationary waves...

Hubble Space Telescope Spots Martian Moon Phobos

Jul 21, 2017 by News Staff

When the NASA/ESA Hubble Space Telescope observed Mars near opposition on May 12, 2016, Phobos — the larger and inner of the two natural satellites...

This image shows Watson 021, a single H7 ordinary chondrite, weighing 135 g. The sample has a large crack, lined with alteration minerals, that runs down its middle and only one third of its fusion crust remains intact. This meteorite shows near complete oxidation of its reduced metal and sulfide phases making this a W4 chondrite. Watson 021 is extensively shocked, exhibiting globular silicate metal emulsions and shock veins that crosscut the sample. Tait et al found that microbial communities in samples of Nullarbor Plain soil are more diverse than those in Watson 021 and other meteorites, which are highly uniform in their species evenness and species richness. Image credit: Tait et al, doi: 10.3389/fmicb.2017.01227.

Research Opens New Way to Understand Possible Martian Life through Meteorites

Jul 20, 2017 by News Staff

New research from Monash University and the University of Queensland has added a new dimension to understanding life on the Red Planet with the discovery...

This image of the Great Red Spot was taken on July 10, 2017, as Juno performed its seventh close flyby of Jupiter. At the time the image was taken, the spacecraft was 8,648 miles (13,917 km) from the tops of the clouds of the planet. Image credit: NASA / SwRI / MSSS.

Juno Captures Close-Up Views of Jupiter’s Great Red Spot

Jul 13, 2017 by News Staff

NASA’s Juno spacecraft has provided planetary researchers the first close-up views of Jupiter’s mysterious, roiling storm called the Great Red Spot. This...

This composite, false-color infrared image of Jupiter reveals haze particles over a range of altitudes, as seen in reflected sunlight. It was taken using the Gemini North telescope’s Near-InfraRed Imager (NIRI) on May 18, 2017. The multiple filters corresponding to each color used in the image cover wavelengths between 1.69 microns and 2.275 microns. Jupiter’s Great Red Spot (GRS) appears as the brightest (white) region at these wavelengths, which are primarily sensitive to high-altitude clouds and hazes near and above the top of Jupiter's convective region. The GRS is one of the highest-altitude features in Jupiter’s atmosphere. Narrow spiral streaks that appear to lead into it or out of it from surrounding regions probably represent atmospheric features being stretched by the intense winds within the GRS, such as the hook-like structure on its western edge (left side). Some are being swept off its eastern edge (right side) and into an extensive wave-like flow pattern, and there is even a trace of flow from its northern edge. Other features near the GRS include the dark block and dark oval to the south and the north of the eastern flow pattern, respectively, indicating a lower density of cloud and haze particles in those locations. Both are long-lived cyclonic circulations, rotating clockwise -- in the opposite direction as the counterclockwise rotation of the GRS. A prominent wave pattern is evident north of the equator, along with two bright ovals, which are anticyclones that appeared in January 2017. Both the wave pattern and the ovals may be associated with an impressive upsurge in stormy activity that has been observed in these latitudes this year. Another bright anticyclonic oval is seen further north. High hazes are evident over both polar regions with much spatial structure not previously been seen quite so clearly in ground-based images. Image credit: Gemini Observatory / AURA / NASA / JPL-Caltech.

Infrared Images of Jupiter from Subaru and Gemini Telescopes to Enhance Juno Flyby

Jul 4, 2017 by News Staff

High-resolution imaging of Jupiter and its Great Red Spot by the Subaru Telescope and the Gemini North telescope, both on Hawaii’s Mauna Kea peak, is...

Georgia Tech researchers propose that a ‘switch-like’ magnetosphere exists at Uranus in both equinox and solstice seasons, where the planetary rotation drives the interchange between an open magnetosphere and a closed magnetosphere each Uranus day. Image credit: NASA / JPL-Caltech.

Uranus Has ‘Switch-Like’ Magnetosphere

Jun 27, 2017 by News Staff

A new study published in the Journal of Geophysical Research: Space Physics suggests that the magnetosphere of the ice giant Uranus gets flipped on and...

A planetary mass object the size of Mars would be sufficient to produce the observed perturbations in the distant Kuiper Belt. Image credit: Heather Roper / Lunar and Planetary Laboratory, University of Arizona.

Mars-to-Earth-Mass Planet May Lurk in Outer Solar System: Planet 10

Jun 22, 2017 by News Staff

An unknown Mars-to-Earth-mass planet may lurk in the outer reaches of the Solar System, according to new research on the orbits of minor planets to be...

The Milky Way Galaxy has a strong preference for two types of planets: rocky planets up to 1.75 times the size of Earth, and gas-enshrouded mini-Neptunes, which are from 2 to 3.5 times the size of Earth. Our Galaxy rarely makes planets with sizes in between these two groups. Image credit: NASA / JPL-Caltech.

Small Exoplanets Come in Two Sizes: Rocky ‘Earths’ and Mini-Neptunes

Jun 20, 2017 by News Staff

Astronomers have classified extrasolar planets in the same way that biologists identify new species and have learned that the majority of planets found...

This artist’s concept shows MAVEN in orbit around Mars, with a fanciful image of Earth in the background. Image credit: NASA / GSFC.

NASA’s MAVEN Mission Celebrates 1,000 Earth Days in Orbit around Mars

Jun 17, 2017 by News Staff

Today, NASA’s Mars Atmosphere and Volatile Evolution (MAVEN) mission — sent to Mars to explore its upper atmosphere, ionosphere and interactions...

Jupiter is the oldest planet in the Solar System. Image credit: NASA.

Jupiter is Solar System’s Oldest Planet, Planetary Researchers Say

Jun 12, 2017 by News Staff

The gas giant Jupiter is not only the most massive planet in our Solar System, but it’s also the oldest, according to an international team of planetary...

The huge storm churning through the atmosphere in Saturn’s northern hemisphere overtakes itself as it encircles the planet in this true-color view from NASA’s Cassini spacecraft. This picture, captured on Feb. 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 planet. Some of the clouds moved south and got caught up in a current that flows to the east (to the right) relative to the storm head. This tail, which appears as slightly blue clouds south and west (left) of the storm head, can be seen encountering the storm head in this view. This storm is the largest, most intense storm observed on Saturn by NASA’s Voyager or Cassini spacecraft. It is still active today. As scientists have tracked this storm over several months, they have found it covers 500 times the area of the largest of the southern hemisphere storms observed earlier in the Cassini mission. The shadow cast by Saturn’s rings has a strong seasonal effect, and it is possible that the switch to powerful storms now being located in the northern hemisphere is related to the change of seasons after the planet’s August 2009 equinox. Image credit: NASA / JPL-Caltech / Space Science Institute.

NASA’s Cassini Orbiter Watches as Saturn’s Solstice Arrives

May 30, 2017 by News Staff

Saturn’s solstice — the longest day of summer in the northern hemisphere and the shortest day of winter in the southern hemisphere — arrived...

Artist’s impression of the Jovian aurora. Image credit: JAXA.

NASA’s Juno Mission Delivers Preliminary Science Results

May 26, 2017 by News Staff

NASA’s Juno mission is rewriting what planetary researchers thought they knew about Jupiter, the largest and most massive planet in our Solar System:...

This artwork shows a rocky planet being bombarded by comets. Image credit: NASA / JPL-Caltech.

Comets Contributed to Earth’s Atmosphere, Says New Study

May 22, 2017 by News Staff

According to new research, some of Earth’s atmosphere was brought to the planet by comets billions of years ago. This artwork shows a rocky planet being...

The young Mars would have had enough water to cover its entire surface in a liquid layer about 140 m deep, but it is more likely that the liquid would have pooled to form an ocean occupying almost half of Mars’s northern hemisphere, and in some regions reaching depths greater than 1.6 km. Image credit: M. Kornmesser / ESO / N. Risinger, skysurvey.org.

Research Reveals How Changes in Rainfall Shaped Early Mars

May 16, 2017 by News Staff

Heavy rain on Mars reshaped impact craters and carved out river-like channels in the planet’s surface billions of years ago, according to a study by...

The atmosphere of the Neptune-mass exoplanet HAT-P-26b is unexpectedly primitive, composed primarily of hydrogen and helium. By combining observations from Hubble and Spitzer space telescopes, Wakeford et al determined that, unlike Neptune and Uranus, the exoplanet has relatively low metallicity. Image credit: NASA’s Goddard Space Flight Center.

HAT-P-26b: Unexpectedly Primitive Atmosphere Discovered around Neptune-Mass Exoplanet

May 12, 2017 by News Staff

Astronomers have discovered that HAT-P-26b — a ‘warm Neptune’ orbiting a dwarf star approximately 437 light-years from Earth — has an atmosphere...

This artist’s impression displays TRAPPIST-1 and its planets reflected in a surface. Image credit: NASA / R. Hurt / T. Pyle.

TRAPPIST-1 System’s Planetary Harmonies Save It from Destruction

May 11, 2017 by News Staff

The recently discovered TRAPPIST-1 planetary system has a unique configuration, according to new research from the University of Toronto, Canada. This...

An artist’s conception of SIMP0136, a planetary-like member of the 200-million-year-old Carina-Near group. Image credit: NASA / JPL / Jonathan Gagne.

One of Nearest Brown Dwarfs is Actually Free-Floating Giant Planet, Astronomers Say

May 10, 2017 by News Staff

A team of astronomers led by the Carnegie Institution has discovered that what scientists had previously thought was one of the closest brown dwarfs to...

This illustration shows Cassini about to make one of its dives between Saturn and its innermost rings as part of the mission’s Grand Finale. Image credit: NASA / JPL-Caltech.

Dust-Free Region between Saturn and Its Rings Puzzles Cassini Scientists

May 2, 2017 by News Staff

On April 26, 2017, NASA’s Cassini orbiter made its first ‘Grand Finale’ dive through the previously unexplored gap between Saturn and its rings....

Jupiter’s Great Cold Spot (a dark spot). Image credit: Stallard et al.

‘Great Cold Spot’ Discovered in Jupiter’s Upper Atmosphere

Apr 12, 2017 by News Staff

An international team of researchers, led by University of Leicester planetary astronomer Tom Stallard, has detected a localized region of cooling —...

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