Seeing baby stars at every stage of their formation

Observations of the Taurus Molecular Cloud obtained by the Herschel Space Observatory. Image credit: ALMA (ESO/NAOJ/NRAO), Tokuda et al., ESA/Herschel

Stars form from the collapse of dense clouds of gas and dust, which makes it very hard for astronomers to watch the process unfold. Recently the ALMA telescope has revealed a treasure trove of embryonic stars in the Taurus Molecular Cloud, illuminating how baby stars are born.

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Lava Tubes on the Moon and Mars are Really, Really Big. Big Enough to Fit an Entire Planetary Base

The first lava tube skylight discovered on the moon. Image credit: JAXA/SELENE

Could lava tubes on the Moon and Mars play a role in establishing a human presence on those worlds? Possibly, according to a team of researchers. Their new study shows that lunar and Martian lava tubes might be enormous, and easily large enough to accommodate a base.

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Astronomers Think They’ve Found the Neutron Star Remnant From Supernova 1987a

Artist's illustration of SN1987A. Credit: NRAO/AUI/NSF, B. Saxton

In 1987, astronomers witnessed a spectacular event when they spotted a titanic supernova 168,000 light-years away in the Hydra constellation. Designated 1987A (since it was the first supernova detected that year), the explosion was one of the brightest supernova seen from Earth in more than 400 years. The last time was Kepler’s Supernova, which was visible to Earth-bound observers back in 1604 (hence the designation SN 1604).

Since then, astronomers have tried in vain to find the company object they believed to be at the heart of the nebula that resulted from the explosion. Thanks to recent observations and a follow-up study by two international teams of astronomers, new evidence has been provided that support the theory that there is a neutron star at the heart of SN 1604 – which would make it the youngest neutron star known to date.

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InSight’s Mole Is In!

The mole is buried, but might still be stuck. Image Credit: NASA/JPL-Caltech

The InSight lander is making progress on Mars. After many months of struggle and careful adaptation, the InSight lander’s ‘Mole’ is finally into the ground. There’s still more delicate work to be done, and they’re not at operating depth yet. But after such a long, arduous affair, this feels like a victory.

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The Martian Sky Pulses in Ultraviolet Every Night

This is an image of the ultraviolet “nightglow” in the Martian atmosphere. Green and white false colors represent the intensity of ultraviolet light, with white being the brightest. The nightglow was measured at about 70 kilometers (approximately 40 miles) altitude by the Imaging UltraViolet Spectrograph instrument on NASA’s MAVEN spacecraft. A simulated view of the Mars globe is added digitally for context. The image shows an intense brightening in Mars’ nightside atmosphere. The brightenings occur regularly after sunset on Martian evenings during fall and winter seasons, and fade by midnight. The brightening is caused by increased downwards winds which enhance the chemical reaction creating nitric oxide which causes the glow. Credits: NASA/MAVEN/Goddard Space Flight Center/CU/LASP

There’s a surprising phenomenon taking place in Mars’ atmosphere: during the spring and fall seasons on the Red Planet, large areas of the sky pulse in ultraviolet light, exactly three times every night.  

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A magnetar has been discovered throwing off bizarre blasts of radiation. Is this where fast radio bursts come from?

Artist's impression of a magnetar throwing off a seriously impressive blast. Image credit: ESA

Magnetars are the ultimate aggressive star: intense magnetic fields, massive outbursts, the works. We’ve known that magnetars are capable of producing some of the most powerful blasts in the cosmos, but new observations reveal a different kind of radiation: radio waves. This could potentially solve the long-standing puzzle of the origins of the mysterious Fast Radio Bursts.

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Asteroids Somehow Migrated Past Jupiter During the Solar System’s Early History

In baseball, players receive a Gold Glove award if they show outstanding fielding play throughout the course of the season.  Basically, they can’t let any ball get past them when playing in the field.  If a Gold Glove award was handed to planets in our solar system, it would undoubtedly be given to Jupiter.  It has long been thought that the massive gas giant hoovered up all of the asteroids in its vicinity.  In doing so, it would have created two distinct zones of asteroids – those inside it’s orbit and those outside.

Now scientists are starting to cast doubt on such a bifurcated model of the early solar system.  And they’re using hundreds of meteorites to do it.

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Neutron stars of different masses can make a real mess when they collide

An artistic rendering of two neutron stars merging. Credit: NSF/LIGO/Sonoma State/A. Simonnet

When neutron stars collide, they go out with a tremendous bang, fueling an explosion up to a thousand times more powerful than a supernova. But sometimes they go out with a whimper, and a recent suite of simulations is showing why: they turn into a black hole.

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Why Can Black Hole Binaries Have Dramatically Different Masses? Multiple Generations of Mergers

Simulated merger of two black holes. Credit: NASA's Goddard Space Flight Center

On the 12th of April, 2019, the LIGO and Virgo gravitational wave observatories detected the merger of two black holes. Named GW190412, one of the black holes was eight solar masses, while the other was 30 solar masses. On the 14th of August that year, an even more extreme merger was observed, when a 2.5 solar mass object merged with a black hole nearly ten times more massive. These mergers raise fundamental questions about the way black hole mergers happen.

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