Category Astronomy/Space

Missing-link in Planet Evolution found

This is an artist’s impression of the newly discovered object.
Credit: Ko Arimatsu

For the first time ever, astronomers have detected a 1.3 km radius body at the edge of the Solar System. Kilometer sized bodies like the one discovered have been predicted to exist for more than 70 years. These objects acted as an important step in the planet formation process between small initial amalgamations of dust and ice and the planets we see today.

The Edgeworth-Kuiper Belt is a collection of small celestial bodies located beyond Neptune’s orbit. The most famous Edgeworth-Kuiper Belt Object is Pluto. Edgeworth-Kuiper Belt Objects are believed to be remnants left over from the formation of the Solar System...

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New Horizons’ Newest and Best-yet View of Ultima Thule

New Horizons' Newest and Best-Yet View of Ultima Thule
Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

The wonders – and mysteries – of Kuiper Belt object 2014 MU69 continue to multiply as NASA’s New Horizons spacecraft beams home new images of its New Year’s Day 2019 flyby target.

This image, taken during the historic Jan. 1 flyby of what’s informally known as Ultima Thule, is the clearest view yet of this remarkable, ancient object in the far reaches of the solar system – and the first small “KBO” ever explored by a spacecraft.

Obtained with the wide-angle Multicolor Visible Imaging Camera (MVIC) component of New Horizons’ Ralph instrument, this image was taken when the KBO was 4,200 miles (6,700 kilometers) from the spacecraft, at 05:26 UT (12:26 a.m. EST) on Jan...

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Stellar Winds, the Source material for the Universe, are Clumpy

Illustration of a high-mass X-ray binary system made up of a compact, incredibly dense neutron star paired with a massive ‘normal’ supergiant star. New data from NASA’s Chandra X-ray Observatory shows that the neutron star in the high-mass X-ray binary, OAO 1657-415, passed through a dense patch of stellar wind from its companion star, demonstrating the clumpy nature of stellar winds.
Credit: NASA/CXC/M.Weiss

Data recorded by NASA’s Chandra X-ray Observatory of a neutron star as it passed through a dense patch of stellar wind emanating from its massive companion star provide valuable insight about the structure and composition of stellar winds and about the environment of the neutron star itself...

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How to Escape a Black Hole: Simulations provide new clues about powerful Plasma jets

This visualization of a general-relativistic collisionless plasma simulation shows the density of positrons near the event horizon of a rotating black hole. Plasma instabilities produce island-like structures in the region of intense electric current.
Credit: Kyle Parfrey et al./Berkeley Lab

Interplay of twisting magnetic field, ‘negative-energy’ particles. How do black holes purge energy locked up in their rotation, jetting near-light-speed plasmas into space to opposite sides in one of the most powerful displays in the universe? These jets can extend outward for millions of light years.

New simulations led by researchers working at the Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab) and UC Berkeley have combined decades-old theories to provide new insight ...

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