Tag Archive for 'Atmosphere'

In 2012 Cassini spotted a cloud system called the south polar vortex in Titan’s atmosphere at an altitude of about 186 miles. The spacecraft’s instrument has now detected a massive ice cloud below it. This image was taken by Cassini in 2013. Image credit: NASA / JPL-Caltech / Space Science Institute.

Cassini Spots Exotic Ice Cloud in Titan’s Stratosphere

Sep 22, 2016 by News Staff

Cassini mission scientists think the appearance of a cloud of dicyanoacetylene ice in Titan’s stratosphere is explained by ‘solid-state’ chemistry...

In this artist’s conception GJ 1132b circles a red dwarf star. Image credit: Dana Berry.

Nearby Earth-Sized Exoplanet GJ 1132b Might Have Oxygen-Rich Atmosphere

Aug 19, 2016 by News Staff

In this artist’s conception GJ 1132b circles a red dwarf star. Image credit: Dana Berry. GJ 1132b, an extrasolar planet about 1.2 times the size and...

This false-color image from Cassini shows clouds in the atmosphere of Saturn. Image credit: NASA / JPL-Caltech / Space Science Institute / Kevin M. Gill.

Stunning New Cassini Image Shows Saturn’s Clouds

Aug 10, 2016 by Enrico de Lazaro

A new infrared image from NASA’s Cassini orbiter shows enormous clouds in the northern hemisphere of the gas giant Saturn. This false-color image from...

Artist’s concept of the mechanism of heating from the Great Red Spot. Turbulent atmospheric flows above the storm produce both gravity waves and acoustic waves. Gravity waves are much like how a guitar string moves when plucked, while acoustic waves are compressions of the air (sound waves). Heating in the upper atmosphere 500 miles (805 km) above the storm is thought to be caused by a combination of these two wave types ‘crashing’ like ocean waves on a beach. Image credit: Karen Teramura, University of Hawaii at Manoa / James O’Donoghue, Boston University.

Great Red Spot Heats Jupiter’s Upper Atmosphere

Jul 28, 2016 by News Staff

The upper atmosphere above Jupiter’s Great Red Spot – the largest storm in the Solar System – is hundreds of degrees hotter than anywhere...

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

Clouds High in Venus’ Atmosphere Reveal Features on Planet’s Surface

Jul 26, 2016 by News Staff

Using data from ESA’s Venus Express spacecraft, European planetary researchers have shown how weather patterns seen in Venus’ cloud layers are directly...

Strong ‘Electric Wind’ Can Strip Terrestrial Planets of Atmospheres, Oceans

Jun 21, 2016 by News Staff

Solar System’s planet Venus has an ‘electric wind’ strong enough to remove the components of water from its upper atmosphere. This action may have...

Radio image (top), made with the VLA, and optical image (bottom) made with the NASA/ESA Hubble Space Telescope, of Jupiter’s Great Red Spot. The radio image shows the complex upwellings and downwellings of ammonia gas 18-56 miles (30-90 km) below the visible clouds. Image credit: Imke de Pater et al / NRAO / AUI / NSF / NASA / ESA.

VLA Radio Maps Reveal What’s Beneath Jupiter’s Thick Clouds

Jun 3, 2016 by News Staff

Scientists using the Karl G. Jansky Very Large Array (VLA) at the National Radio Astronomy Observatory have produced detailed radio maps of Jupiter’s...

Ancient Earth. Image credit: Imperial College London.

Archean Earth’s Upper Atmosphere Was Oxygen-Rich, Scientists Discover

May 12, 2016 by News Staff

An international team of researchers from Australia and the United Kingdom has made a surprising discovery about the chemistry of Earth’s upper atmosphere...

SOFIA/GREAT spectrum of oxygen [OI] superimposed on an image of Mars from NASA’ MAVEN mission. The amount of atomic oxygen computed from SOFIA data is about half the amount expected. Image credit: NASA / DLR / USRA / DSI / MPIfR / GREAT Consortium / MPIfS / Rezac et al / MAVEN.

NASA’s SOFIA Observatory Detects Atomic Oxygen in Upper Atmosphere of Mars

May 10, 2016 by Enrico de Lazaro

NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA), the largest airborne observatory in the world, has detected atomic oxygen in the upper...

ESA’s Venus Express Finds Atmospheric Gravity Waves in Venusian Polar Atmosphere

Apr 23, 2016 by News Staff

Strong atmospheric gravity waves dominate the polar regions of Venus’ atmosphere, according to measurements made by ESA’s Venus Express spacecraft...

A solar storm approaches Mars. Image credit: NASA Goddard Space Flight Center.

NASA’s MAVEN Team: Solar Storms Stripped Away Mars’ Atmosphere

Nov 6, 2015 by News Staff

Thanks to NASA’s Mars Atmosphere and Volatile Evolution (MAVEN) orbiter, scientists have learned more about what happened to the Martian climate since...

According to NASA scientists, complex chemical compounds called tholins give Pluto a distinctive blue haze. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute.

Latest New Horizons Image Shows Pluto’s ‘Blue Skies’

Oct 9, 2015 by News Staff

NASA’s New Horizons spacecraft has beamed back the first color image of Pluto’s atmosphere. New Horizons looks toward the night side of Pluto and sees...

This false-color image shows carbon nanofibers. Image credit: Stuart Licht.

Scientists Turn Atmospheric Carbon Dioxide into Nanofibers

Aug 20, 2015 by News Staff

A group of researchers led by Dr Stuart Licht of George Washington University has developed a novel method to economically convert atmospheric carbon dioxide...

This mosaic provides the best view ever obtained of the dwarf planet Pluto. The lower right edge of the planet in this view currently lacks high-resolution color coverage. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute.

Pluto’s Atmospheric Nitrogen Likely Has Internal Origin, Scientists Say

Aug 12, 2015 by News Staff

Researchers at Southwest Research Institute are studying the data collected by NASA’s New Horizons spacecraft to discover what is pumping up the nitrogen...

The hazes in Pluto’s atmosphere provide a crucial link between the sunlight-driven chemistry in the upper atmosphere and the reddish-brown hydrocarbons called tholins that rain down and darken the surface. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute.

New Horizons Sheds More Light on Pluto’s Atmosphere

Jul 27, 2015 by News Staff

Just seven hours after closest approach, the spacecraft looked back and captured an incredible image of the dwarf planet’s atmosphere, backlit by the...

Pluto nearly fills the frame in this image from NASA’s New Horizons spacecraft, taken on July 13, 2015, when the spacecraft was 476,000 miles (768,000 km) from the dwarf planet’s surface. This is the last and most detailed image sent to Earth before the spacecraft’s closest approach to Pluto on July 14. The color image has been combined with lower-resolution color information from the Ralph instrument that was acquired earlier on July 13. This view is dominated by the large, bright feature informally named the ‘heart,’ which measures around 1,000 miles (1,600 km) across. The heart’s diameter is about the same distance as from Denver to Chicago, in America’s heartland. The heart borders darker equatorial terrains, and the mottled terrain to its east (right) are complex. However, even at this resolution, much of the heart’s interior appears remarkably featureless-possibly a sign of ongoing geologic processes. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute.

NASA’s New Horizons Uncovers Hidden Secrets of Pluto’s Atmosphere

Jul 20, 2015 by News Staff

The Alice instrument – a lightweight (4.4 kg), low-power (4.4 Watt) imaging spectrograph aboard NASA’s New Horizons – has observed Pluto’s...

Map of MAVEN’s auroral detections in December 2014 overlaid on the surface of Mars: the map shows that the aurora was widespread in the northern hemisphere, not tied to any geographic location. Image credit: University of Colorado.

MAVEN Sheds New Light on Atmosphere of Mars

Jun 24, 2015 by News Staff

NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) spacecraft has observed three phenomena in the atmosphere of Mars: a polar plume of escaping atmospheric...

Small pollen particles can hold condensation for cloud formation. Image credit: Brin Weins.

Pollen Grains Can Influence Climate, Scientists Say

May 6, 2015 by News Staff

According to a team of researchers led by Prof Allison Steiner of the University of Michigan, tiny pollen particles may make it rain. Small pollen particles...

A hypothetical mini-Neptune. Image credit: DLR Institute of Planetary Research.

Astronomers Discover Brightly Illuminated mini-Neptune

May 4, 2015 by News Staff

A group of astronomers led by Benjamin Montet of the California Institute of Technology, Pasadena, has discovered a highly irradiated mini-Neptune exoplanet...

Dr Martin Vollmer and his colleagues detected a rapid accumulation of anesthetic gases isoflurane, desflurane, and sevoflurane, in the global atmosphere. Image credit: NASA Goddard Space Flight Center.

Anesthetic Gases Contribute to Climate Change, Say Atmospheric Chemists

Apr 9, 2015 by News Staff

Desflurane, isoflurane, sevoflurane and halothane – clinically used inhalation anesthetic agents – are accumulating in the atmosphere of our...

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