Category Astronomy/Space

Secrets behind Pluto’s Dunes revealed

This image taken during the New Horizons mission shows the mountain range on the edge of the Sputnik Planitia ice plain, with dune formations clearly visible in the bottom half of the picture. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

This image taken during the New Horizons mission shows the mountain range on the edge of the Sputnik Planitia ice plain, with dune formations clearly visible in the bottom half of the picture. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

Scientists have discovered dunes on Pluto, and say they are likely to have been formed of methane ice grains released into its rarefied atmosphere. Writing in Science, an international team of geographers, physicists and planetary scientists have analysed detailed images of the dwarf planet’s surface, captured in July 2015 by NASA’s New Horizons spacecraft...

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XENON1T experimental data establishes most stringent Limit on Dark Matter

Experimental results from the XENON1T dark matter detector limit the effective size of dark matter particles to 4.1X10-47 square centimeters--one-trillionth of one-trillionth of a centimeter squared--the most stringent limit yet determined for dark matter as established by the world's most sensitive detector. Credit: XENON Collaboration

Experimental results from the XENON1T dark matter detector limit the effective size of dark matter particles to 4.1X10-47 square centimeters–one-trillionth of one-trillionth of a centimeter squared–the most stringent limit yet determined for dark matter as established by the world’s most sensitive detector. Credit: XENON Collaboration

Analysis scours 276 days of data from world’s most sensitive detector. Experimental results from the XENON1T dark matter detector limit the effective size of dark matter particles to 4.1 x 10-47 square centimeters – one-trillionth of one-trillionth of a centimeter squared – the most stringent limit yet determined for dark matter as established by the world’s most sensitive detector.

The results, presented Monday in a seminar in Italy at the Gran Sasso Undergr...

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Large Magellanic Cloud: A crowded neighborhood

Glowing brightly about 160,000 light-years away, the Tarantula Nebula is the most spectacular feature of the Large Magellanic Cloud, a satellite galaxy to our Milky Way. This image from VLT Survey Telescope at ESO's Paranal Observatory in Chile shows the region and its rich surroundings in great detail. It reveals a cosmic landscape of star clusters, glowing gas clouds and the scattered remains of supernova explosions. Credit: ESO

Glowing brightly about 160,000 light-years away, the Tarantula Nebula is the most spectacular feature of the Large Magellanic Cloud, a satellite galaxy to our Milky Way. This image from VLT Survey Telescope at ESO’s Paranal Observatory in Chile shows the region and its rich surroundings in great detail. It reveals a cosmic landscape of star clusters, glowing gas clouds and the scattered remains of supernova explosions. Credit: ESO

Glowing brightly about 160,000 light-years away, the Tarantula Nebula is the most spectacular feature of the Large Magellanic Cloud, a satellite galaxy to our Milky Way. A new image reveals a cosmic landscape of star clusters, glowing gas clouds and the scattered remains of supernova explosions. This is the sharpest image ever of this entire field.

Taking advanta...

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The Case of the Relativistic Particles Solved with NASA Missions

In a background magnetic field, represented by the cyan arrows, two electrons are propagating to the right, executing identical gyromotion. A circularly polarized electromagnetic wave approaches the upper electron from the left. Credits: NASA

In a background magnetic field, represented by the cyan arrows, two electrons are propagating to the right, executing identical gyromotion. A circularly polarized electromagnetic wave approaches the upper electron from the left.
Credits: NASA

Encircling Earth are two enormous rings – Van Allen radiation belts – of highly energized ions and electrons. Various processes can accelerate these particles to relativistic speeds, which endanger spacecraft unlucky enough to enter these giant bands of damaging radiation. Scientists had previously identified certain factors that might cause particles in the belts to become highly energized, but they had not known which cause dominates.

Now, with new research from NASA’s Van Allen Probes and Time History of Events and Macroscale Interactions during Sub...

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