Category Astronomy/Space

NASA Protects its Super Heroes from Space Weather

NASA's Human Research Program aims to mitigate the harmful effects of the space radiation environment on astronaut health outside of the relative protection of the Earth's magnetosphere. Credit: NASA/SOHO

NASA’s Human Research Program aims to mitigate the harmful effects of the space radiation environment on astronaut health outside of the relative protection of the Earth’s magnetosphere. Credit: NASA/SOHO

NASA’s Human Research Program (HRP) is studying the effects radiation plays on the human body and developing ways to monitor and protect against this silent hazard. High-energy galactic cosmic rays (GCRs) which are remnants from supernovas and solar storms like solar particle events (SPEs) and coronal mass ejections (CMEs) from the sun can cause harm to the body and spacecraft. These are all components of space weather

“Dosimeters and modeling techniques are used to determine how much energy is deposited in the space explorer’s bodies along with inflight tools to try to estimate what type...

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Supermassive black holes feed on Cosmic Jellyfish

Observations of 'Jellyfish galaxies' with ESO's Very Large Telescope have revealed a previously unknown way to fuel supermassive black holes. It seems the mechanism that produces the tentacles of gas and newborn stars that give these galaxies their nickname also makes it possible for the gas to reach the central regions of the galaxies, feeding the black hole that lurks in each of them and causing it to shine brilliantly. This picture of one of the galaxies, nicknamed JO204, from the MUSE instrument on ESO's Very Large Telescope in Chile, shows clearly how material is streaming out of the galaxy in long tendrils to the lower-left. Red shows the glow from ionised hydrogen gas and the whiter regions are where most of the stars in the galaxy are located. Some more distant galaxies are also visible. Credit: ESO/GASP collaboration; CC-BY; Creative Commons Attribution 4.0 International License

Observations of ‘Jellyfish galaxies’ with ESO’s Very Large Telescope have revealed a previously unknown way to fuel supermassive black holes. It seems the mechanism that produces the tentacles of gas and newborn stars that give these galaxies their nickname also makes it possible for the gas to reach the central regions of the galaxies, feeding the black hole that lurks in each of them and causing it to shine brilliantly. This picture of one of the galaxies, nicknamed JO204, from the MUSE instrument on ESO’s Very Large Telescope in Chile, shows clearly how material is streaming out of the galaxy in long tendrils to the lower-left. Red shows the glow from ionised hydrogen gas and the whiter regions are where most of the stars in the galaxy are located...

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Cosmic Magnifying Lens reveals Inner Jets of Black Holes

Illustration shows a likely configuration of a gravitational lensing system discovered by OVRO. The 'milli-lens' is located in or near the intervening spiral galaxy. The lens is magnifying blobs of jet material within the active galaxy PKS1413+135, but the blobs are too small to be seen in the radio image (top left), taken by MOJAVE. Only when the blobs move far away from the yellow core do they expand and are visible as the pink blobs in the image. Credit: Anthony Readhead/Caltech/MOJAVE

Illustration shows a likely configuration of a gravitational lensing system discovered by OVRO. The ‘milli-lens’ is located in or near the intervening spiral galaxy. The lens is magnifying blobs of jet material within the active galaxy PKS1413+135, but the blobs are too small to be seen in the radio image (top left), taken by MOJAVE. Only when the blobs move far away from the yellow core do they expand and are visible as the pink blobs in the image. Credit: Anthony Readhead/Caltech/MOJAVE

New radio observations show clumps of gas streaming from supermassive black hole...

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Cosmic Velocity Web: Motions of Thousands of Galaxies Mapped

The cosmic velocity web is represented by surfaces of knots in red and surfaces of filaments in gray. The black lines with arrows illustrate local velocity flows within filaments and toward knots. The Laniakea Supercluster basin of attraction that includes our Milky Way galaxy is represented by a blue surface. The region being displayed extends across one billion light years. Credit: Daniel Pomarede, Yehuda Hoffman, R. Brent Tully and Helene Courtois. Credit: Daniel Pomarede, Yehuda Hoffman, R. Brent Tully, Helene Courtois

The cosmic velocity web is represented by surfaces of knots in red and surfaces of filaments in gray. The black lines with arrows illustrate local velocity flows within filaments and toward knots. The Laniakea Supercluster basin of attraction that includes our Milky Way galaxy is represented by a blue surface. The region being displayed extends across one billion light years. Credit: Daniel Pomarede, Yehuda Hoffman, R. Brent Tully and Helene Courtois. Credit: Daniel Pomarede, Yehuda Hoffman, R. Brent Tully, Helene Courtois

The cosmic web – the distribution of matter on the largest scales in the universe – has usually been defined through the distribution of galaxies. Now, a new study by a team of astronomers from France, Israel and Hawaii demonstrates a novel approach...

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