Category Astronomy/Space

First Observations ever of the Outskirts of a Supermassive Black Hole’s Accretion Disk

An artist’s impression of a supermassive black hole with an accretion disk orbiting it. The annotations show a hypothetical double-peaked profile with arrows indicating where in the broad line region each peak originates. Credit: NOIRLab/NSF/AURA/P. Marenfeld
An artist’s impression of a supermassive black hole with an accretion disk orbiting it. The annotations show a hypothetical double-peaked profile with arrows indicating where in the broad line region each peak originates. Credit: NOIRLab/NSF/AURA/P. Marenfeld

Nothing can evoke an existential perspective-spiral quite like looking at an image of a galaxy. At first glance, these sublime structures may appear rather serene. But in fact the center of many galaxies is a turbulent environment containing an actively feeding supermassive black hole.

Orbiting these incomprehensibly dense objects are swirling accretion disks of gas and dust, which feed the black hole and emit copious amounts of energy all along the electromagnetic spectrum—from high-energy gamma rays and X-rays, through visi...

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Mysterious Neptune Dark Spot detected from Earth for the first time

There are four telescopic images of the planet Neptune side-by-side. The rightmost one is an almost-featureless cyan disc with a faint dark spot to the upper-right. The other three, coloured in blue, green and red, show higher contrast views of dark and bright spots, as well as bands crossing the planet diagonally.

Using ESO’s Very Large Telescope (VLT), astronomers have observed a large dark spot in Neptune’s atmosphere, with an unexpected smaller bright spot adjacent to it. This is the first time a dark spot on the planet has ever been observed with a telescope on Earth. These occasional features in the blue background of Neptune’s atmosphere are a mystery to astronomers, and the new results provide further clues as to their nature and origin.

Large spots are common features in the atmospheres of giant planets, the most famous being Jupiter’s Great Red Spot. On Neptune, a dark spot was first discovered by NASA’s Voyager 2 in 1989, before disappearing a few years later...

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European Astronomers Detect New Component of Radio Halo in a Nearby Galaxy Cluster

European astronomers detect new component of radio halo in a nearby galaxy cluster
Composite RGB image of Abell 2142: radio (GMRT, 323 MHz) in red, optical (DSS-2, red filter) in green, and X-rays (XMM-Newton) in blue. Credit: Bruno et al., 2023.

Using the LOw Frequency ARray (LOFAR), astronomers from the University of Bologna, Italy and elsewhere, have conducted radio observations of the nearby galaxy cluster Abell 2142. In result, they detected a new component of the cluster’s giant radio halo. The finding was presented in a paper published August 15 on the pre-print server arXiv.

Galaxy clusters contain up to thousands of galaxies bound together by gravity. They are the largest known gravitationally bound structures in the universe, and could serve as excellent laboratories for studying galaxy evolution and cosmology.

Radio halos are enormous regions of diff...

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Penetrating Radar Aboard the Chang’E-4 Rover Reveals Layers of the Moon’s History

Penetrating radar aboard the Chang'E-4 rover reveals layers of the moon's history
Image taken by the panoramic camera (PCAM) on board the Chinese Yutu 2 lunar rover as it looked back at the Chang’e 4 lander. Credit: Nature Communications (2019). DOI: 10.1038/s41467-019-12278-3/Wikimedia Commons/CC BY-SA

A team of space scientists at the Planetary Science Institute, working with colleagues from the Chinese Academy of Sciences, Shenzhen University and the University of Aberdeen, has used data from China’s Chang’E-4 rover to learn more about the history of the moon. In their study, reported in the Journal of Geophysical Research: Planets, the group analyzed lunar-penetrating radar (LPR) data sent back from the rover.

China’s Chang’E-4 rover has been wandering around on the far side of the moon since 2018...

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