Clarksville, TN Online: News, Opinion, Arts & Entertainment.


Topic: Mercury

NASA’s MESSENGER Spacecraft data shows how Micrometeoroids effect Mercury’s Atmosphere

 

Written by Kathryn DuFresne
NASA’s Goddard Space Flight Center

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – Mercury, our smallest planetary neighbor, has very little to call an atmosphere, but it does have a strange weather pattern: morning micro-meteor showers.

Recent modeling along with previously published results from NASA’s MESSENGER spacecraft — short for Mercury Surface, Space Environment, Geochemistry and Ranging, a mission that observed Mercury from 2011 to 2015 — has shed new light on how certain types of comets influence the lopsided bombardment of Mercury’s surface by tiny dust particles called micrometeoroids. This study also gave new insight into how these micrometeoroid showers can shape Mercury’s very thin atmosphere, called an exosphere. 

Scientists used models along with earlier findings from the MESSENGER mission to shed light on how certain types of comets influence the micrometeoroids that preferentially impact Mercury on the dawn side of the planet. Here, data from the Mercury Atmosphere and Surface Composition Spectrometer, or MASCS, instrument is overlain on the mosaic from the Mercury Dual Imaging System, or MDIS. (NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington)

Scientists used models along with earlier findings from the MESSENGER mission to shed light on how certain types of comets influence the micrometeoroids that preferentially impact Mercury on the dawn side of the planet. Here, data from the Mercury Atmosphere and Surface Composition Spectrometer, or MASCS, instrument is overlain on the mosaic from the Mercury Dual Imaging System, or MDIS. (NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington)

«Read the rest of this article»

Sections: Technology | No Comments
 

NASA to chase Total Solar Eclipse from WB-57F Jets

 

Written by Mara Johnson-Groh
NASA’s Goddard Space Flight Center

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – For most viewers, the Monday, August 21st, 2017, total solar eclipse will last less than two and half minutes. But for one team of NASA-funded scientists, the eclipse will last over seven minutes. Their secret? Following the shadow of the Moon in two retrofitted WB-57F jet planes.

Amir Caspi of the Southwest Research Institute in Boulder, Colorado, and his team will use two of NASA’s WB-57F research jets to chase the darkness across America on August 21st. Taking observations from twin telescopes mounted on the noses of the planes, Caspi will ­­­­­capture the clearest images of the Sun’s outer atmosphere — the corona — to date and the first-ever thermal images of Mercury, revealing how temperature varies across the planet’s surface.

(Photo illustration) During the upcoming total solar eclipse, a team of NASA-funded scientists will observe the solar corona using stabilized telescopes aboard two of NASA’s WB-57F research aircraft. This vantage point provides distinct advantages over ground-based observations, as illustrated by this composite photo of the aircraft and the 2015 total solar eclipse at the Faroe Islands. (NASA/Faroe Islands/SwRI)

(Photo illustration) During the upcoming total solar eclipse, a team of NASA-funded scientists will observe the solar corona using stabilized telescopes aboard two of NASA’s WB-57F research aircraft. This vantage point provides distinct advantages over ground-based observations, as illustrated by this composite photo of the aircraft and the 2015 total solar eclipse at the Faroe Islands. (NASA/Faroe Islands/SwRI)

«Read the rest of this article»

Sections: Technology | No Comments
 

NASA’s Dawn mission reveals Ceres’ Ice in Shadowed Craters related to dwarf planet’s tilt

 

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Dwarf planet Ceres may be hundreds of millions of miles from Jupiter, and even farther from Saturn, but the tremendous influence of gravity from these gas giants has an appreciable effect on Ceres’ orientation.

In a new study, researchers from NASA’s Dawn mission calculate that the axial tilt of Ceres — the angle at which it spins as it journeys around the sun — varies widely over the course of about 24,500 years. Astronomers consider this to be a surprisingly short period of time for such dramatic deviations.

This animation shows how the illumination of Ceres' northern hemisphere varies with the dwarf planet's axial tilt, or obliquity. Shadowed regions are highlighted for tilts of 2 degrees, 12 degrees and 20 degrees. (NASA/JPL-Caltech/UCLA/MPS/DLR/IDA)

This animation shows how the illumination of Ceres’ northern hemisphere varies with the dwarf planet’s axial tilt, or obliquity. Shadowed regions are highlighted for tilts of 2 degrees, 12 degrees and 20 degrees. (NASA/JPL-Caltech/UCLA/MPS/DLR/IDA)

«Read the rest of this article»

Sections: Technology | No Comments
 


NASA researchers say Mars may have had Rings

 

Written by Brian Wallheimer
NASA Headquarters

NASA - National Aeronautics and Space AdministrationWashington, D.C. – As children, we learned about our solar system’s planets by certain characteristics — Jupiter is the largest, Saturn has rings, Mercury is closest to the sun. Mars is red, but it’s possible that one of our closest neighbors also had rings at one point and may have them again someday.

That’s the theory put forth by NASA-funded scientists at Purdue University, Lafayette, Indiana, whose findings were published in the journal Nature Geoscience. David Minton and Andrew Hesselbrock developed a model that suggests that debris that was pushed into space from an asteroid or other body slamming into Mars around 4.3 billion years ago alternates between becoming a planetary ring and clumping together to form a moon.

This sequence of images from NASA's Curiosity Mars rover shows one of Mars' two moons, Phobos, passing directly in front of the other, Deimos, in 2013. (NASA/JPL-Caltech/Malin Space Science Systems/Texas A&M Univ.)

This sequence of images from NASA’s Curiosity Mars rover shows one of Mars’ two moons, Phobos, passing directly in front of the other, Deimos, in 2013. (NASA/JPL-Caltech/Malin Space Science Systems/Texas A&M Univ.)

«Read the rest of this article»

Sections: Technology | No Comments
 

NASA prepares Satellites for alignment of Planets and Stars

 

Written by Mara Johnson-Groh
NASA’s Goddard Space Flight Center

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – The movements of the stars and the planets have almost no impact on life on Earth, but a few times per year, the alignment of celestial bodies has a visible effect.

One of these geometric events — the spring equinox — is just around the corner, and another major alignment — a total solar eclipse — will be visible across America on August 21st, with a fleet of NASA satellites viewing it from space and providing images of the event.

To understand the basics of celestial alignments, here is information on equinoxes, solstices, full moons, eclipses and transits:

During a transit, a planet passes in between us and the star it orbits. This method is commonly used to find new exoplanets in our galaxy. (NASA's Goddard Space Flight Center/Genna Duberstein)

During a transit, a planet passes in between us and the star it orbits. This method is commonly used to find new exoplanets in our galaxy. (NASA’s Goddard Space Flight Center/Genna Duberstein)

«Read the rest of this article»

Sections: Technology | No Comments
 

NASA’s Dawn spacecraft reveals new areas where Ice may hide on Ceres

 

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – At first glance, Ceres, the largest body in the main asteroid belt, may not look icy. Images from NASA’s Dawn spacecraft have revealed a dark, heavily cratered world whose brightest area is made of highly reflective salts — not ice.

But newly published studies from Dawn scientists show two distinct lines of evidence for ice at or near the surface of the dwarf planet. Researchers are presenting these findings at the 2016 American Geophysical Union meeting in San Francisco.

This graphic shows a theoretical path of a water molecule on Ceres. Some water molecules fall into cold, dark craters called "cold traps," where very little of the ice turns into vapor, even over the course of a billion years. (NASA/JPL-Caltech/UCLA/MPS/DLR/IDA)

This graphic shows a theoretical path of a water molecule on Ceres. Some water molecules fall into cold, dark craters called “cold traps,” where very little of the ice turns into vapor, even over the course of a billion years. (NASA/JPL-Caltech/UCLA/MPS/DLR/IDA)

«Read the rest of this article»

Sections: Technology | No Comments
 

NASA’s MESSENGER spacecraft finds Great Valley on Mercury

 

NASA

NASA - National Aeronautics and Space AdministrationWashington, D.C. – A newly discovered “great valley” in the southern hemisphere of Mercury provides more evidence that the small planet closest to the sun is shrinking.

Scientists used stereo images from NASA’s MESSENGER spacecraft to create a high-resolution topo map that revealed the broad valley — more than 620 miles (1,000 kilometers) long — extending into the Rembrandt basin, one of the largest and youngest impact basins on Mercury. About 250 miles (400 kilometers) wide and 2 miles (3 kilometers) deep, Mercury’s great valley is smaller than Mars’ Valles Marineris, but larger than North America’s Grand Canyon and wider and deeper than the Great Rift Valley in East Africa.

Using colorized topography, Mercury’s “great valley” (dark blue) and Rembrandt impact basin (purple, upper right) are revealed in this high-resolution digital elevation model merged with an image mosaic obtained by NASA’s MESSENGER spacecraft.(NASA/JHUAPL/Carnegie Institution of Washington/DLR/Smithsonian Institution)

Using colorized topography, Mercury’s “great valley” (dark blue) and Rembrandt impact basin (purple, upper right) are revealed in this high-resolution digital elevation model merged with an image mosaic obtained by NASA’s MESSENGER spacecraft.(NASA/JHUAPL/Carnegie Institution of Washington/DLR/Smithsonian Institution)

«Read the rest of this article»

Sections: Technology | No Comments
 


NASA’s Cassini mission works to determine the length of a Saturn Day

 

Written by Jay Thompson
Cassini Public Engagement, NASA-JPL

NASA - National Aeronautics and Space AdministrationPasadena, CA – Humans sometimes struggle to adjust to Daylight Saving Time, but just measuring the exact length of a Saturn day is one of the big challenges for scientists on NASA’s Cassini mission. Over more than a decade in Saturn orbit, Cassini’s instruments have wrestled with confusing measurements to determine the planet’s precise rotation rate.

The mission’s final year and unprecedented trajectory will carry Cassini to unexplored regions so near to Saturn that scientists might finally answer the question:

Just how long is a day on Saturn?

Saturn as seen by NASA's Cassini spacecraft in 2008. Long-term tracking of the spacecraft's position has revealed no unexplained perturbations in Cassini's orbit. (NASA/JPL/Space Science Institute)

Saturn as seen by NASA’s Cassini spacecraft in 2008. Long-term tracking of the spacecraft’s position has revealed no unexplained perturbations in Cassini’s orbit. (NASA/JPL/Space Science Institute)

«Read the rest of this article»

Sections: Technology | No Comments
 

NASA says Star Trek’s Vulcan may not exist, but Spock’s home system “40 Eridani” is real

 

NASA Headquarters

NASA - National Aeronautics and Space AdministrationWashington, D.C. – It takes a little imagination to wish some favorite fictional universes into existence. But, for legions of “Star Trek” fans, they don’t have to wish: one star system really exists in our Milky Way galaxy.

In Star Trek lore, Vulcan is the home of logic, learning and the deeply beloved first officer Mr. Spock. While Vulcan is fictional, the star system it belongs to–40 Eridani–is very real. It’s located only 16.5 light-years away from Earth and its primary star can be spotted with the naked eye.

The green area surrounding 40 Eridani A depicts the habitable zone of the star, the area where temperatures would be right for liquid water, an essential ingredient for life (Vulcan or otherwise). The habitable zone of Vulcan is closer to its dwarf star than the Earth's is to the sun because 40 Eridani A is cooler and dimmer than our sun. (NASA)

The green area surrounding 40 Eridani A depicts the habitable zone of the star, the area where temperatures would be right for liquid water, an essential ingredient for life (Vulcan or otherwise). The habitable zone of Vulcan is closer to its dwarf star than the Earth’s is to the sun because 40 Eridani A is cooler and dimmer than our sun. (NASA)

«Read the rest of this article»

Sections: Technology | No Comments
 

NASA’s Dawn Mission identifies Craters on Ceres where Ice could be trapped

 

Written by Elizabeth Zubritsky
NASA’s Goddard Space Flight Center

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – Scientists with NASA’s Dawn mission have identified permanently shadowed regions on the dwarf planet Ceres. Most of these areas likely have been cold enough to trap water ice for a billion years, suggesting that ice deposits could exist there now.

“The conditions on Ceres are right for accumulating deposits of water ice,” said Norbert Schorghofer, a Dawn guest investigator at the University of Hawaii at Manoa. “Ceres has just enough mass to hold on to water molecules, and the permanently shadowed regions we identified are extremely cold — colder than most that exist on the moon or Mercury.”

At the poles of Ceres, scientists have found craters that are permanently in shadow (indicated by blue markings). Such craters are called "cold traps" if they remain below about minus 240 degrees Fahrenheit (minus 151 degrees Celsius). (NASA/JPL-Caltech/UCLA/MPS/DLR/IDA)

At the poles of Ceres, scientists have found craters that are permanently in shadow (indicated by blue markings). Such craters are called “cold traps” if they remain below about minus 240 degrees Fahrenheit (minus 151 degrees Celsius). (NASA/JPL-Caltech/UCLA/MPS/DLR/IDA)

«Read the rest of this article»

Sections: Technology | No Comments
 


Page 1 of 812345...»

  • Visit Us On FacebookVisit Us On TwitterVisit Us On GooglePlusVisit Us On PinterestVisit Us On YoutubeCheck Our Feed
  • Personal Controls

    Archives