Astronomy Archives

October 19, 2020October 19, 2020 by Ralph Crewe

You’ll Experience 200 Times More Radiation Standing on the Moon than Standing on the Earth

Image of the lunar surface taken by the Chang'e-4 spacecraft. Credit: Xinhua

January 31, 2021, will mark 50 years since the launch of Apollo 14. This historic mission was the first to broadcast a color television signal from the surface of the Moon and marked the heroic return to space of America’s first astronaut, Alan Shepard, who famously hit two golf balls off of the lunar regolith. While the significance of Apollo 14 and the Apollo program, in general, can’t be overstated, Shepard spent a mere two days on the lunar surface. The record for the longest human presence on the Moon, held by Eugene Cernan and Harrison Schmitt, is just over three days. All of the Apollo astronauts were exposed to high levels of radiation on the surface of the Moon but with such relatively short stays, the risk was considered to be acceptable.

October 19, 2020October 19, 2020 by Matt Williams

What’s Happening with Betelgeuse? Astronomers Propose a Specialized Telescope to Watch the Star Every Night

Artist's impression of Betelgeuse. Credit: ESO/L. Calçada

Starting in late 2019, Betelgeuse began drawing a lot of attention after it mysteriously started dimming, only to brighten again a few months later. For a variable star like Betelgeuse, periodic dimming and brightening are normal, but the extent of its fluctuation led to all sorts of theories as to what might be causing it. Similar to Tabby’s Star in 2015, astronomers offered up the usual suspects (minus the alien megastructure theory!)

Whereas some thought that the dimming was a prelude to the star becoming a Type II supernova, others suggested that dust clouds, enormous sunspots, or ejected clouds of gas were the culprit. In any case, the “Great Dimming of Betelgeuse” has motivated an international team of astronomers to propose that a “Betelgeuse Scope” be created that cant monitor the star constantly.

October 14, 2020October 14, 2020 by Matt Williams

The Most Comprehensive 3D Map of Galaxies Has Been Released

Credit: Danny Farrow, Pan-STARRS1 Science Consortium and Max Planck Institute for Extraterrestrial Physics

Atop the summit of Haleakala on the Hawaiian island of Maui sits the Panoramic Survey Telescope and Rapid Response System, or Pan-STARRS1 (PS1). As part of the Haleakala Observatory overseen by the University of Hawaii, Pan-STARRS1 relies on a system of cameras, telescopes, and a computing facility to conduct an optical imaging survey of the sky, as well as astrometry and photometry of know objects.

In 2018, the University of Hawaii at Manoa’s Institute for Astronomy (IfA) released the PS1 3pi survey, the world’s largest digital sky survey that spanned three-quarters of the sky and encompassed 3 billion objects. And now, a team of astronomers from the IfA have used this data to create the Pan-STARRS1 Source Types and Redshifts with Machine Learning (PS1-STRM), the world’s largest three-dimensional astronomical catalog.

October 14, 2020October 15, 2020 by David Dickinson

BepiColombo Mercury Mission to Make First Venus Flyby Tonight

The Mercury-bound BepiColombo spacecraft will observe Venus during tonight’s pass, on the hunt for phosphine and sulfur-dioxide.

The joint Japanese/European Space Agency’s BepiColombo spacecraft makes a scheduled pass near Venus tonight, while the cloud-shrouded planet has been very much in the news.

October 14, 2020October 14, 2020 by Evan Gough

We’re Made of Starstuff. Especially From Extremely Massive Stars

An illustration of a protoplanetary disk. The solar system formed from such a disk. Astronomers suggest this birthplace was protected by a larger filament of molecular gas and dust early in history. Credit: NASA/JPL-Caltech/T. Pyle (SSC)

A new study shows how massive young stars create the kind of organic molecules that are necessary for life.

A team of researchers used an airborne observatory to examine the inner regions around two massive young stars. Along with water, they found things like ammonia and methane. These molecules are swirling around in a disk of material that surrounds the young stars.

That material is the same stuff that planets form from, and the study presents some new insights into how the stuff of life becomes incorporated into planets.

October 13, 2020October 16, 2020 by Paul M. Sutter

Do Ripples on the Surface of the Sun tell us that a Flare is Coming?

Flares from the sun are some of the nastiest things in the solar system. When the sun flares, it belches out intense X-ray radiation (and sometimes even worse). Predicting solar flares is a tricky job, and a new research paper sheds light on a possible new technique: looking for telltale ripples in the surface of the sun minutes before the blast comes.

October 13, 2020October 13, 2020 by Evan Gough

An Exoplanet So Hot There Are 7 Different Kinds of Gaseous Metals in its Atmosphere

This artist's illustration shows an alien world that is losing magnesium and iron gas from its atmosphere. The observations represent the first time that so-called "heavy metals"—elements more massive than hydrogen and helium—have been detected escaping from a hot Jupiter, a large gaseous exoplanet orbiting very close to its star. The planet, known as WASP-121b, orbits a star brighter and hotter than the Sun. Image Credit: NASA, ESA, and J. Olmsted (STScI)

The search for exoplanets has revealed types of planets that are nothing like the worlds in our own Solar System. One such type is the hot-Jupiter. They’re gas giants like Jupiter that orbit their host star very closely. That proximity raises their temperatures to extreme heights.

Hot-Jupiters can be hot enough to vaporize metals, making their atmospheres un-Earthlike. A team of astronomers examining one exoplanet has found 7 different gaseous metals in its atmosphere.

October 13, 2020October 14, 2020 by David Dickinson

Comet P1 NEOWISE Makes a Brief Late October Appearance

Comet P1 NEOWISE will make a brief dawn appearance for northern hemisphere observers in late October/early November.

So, how about Comet F3 NEOWISE this summer? 2020 saw the rapid appearance of one of the best northern hemisphere comets in recent memory, and the first good comet for us up north for the 21^st century, as F3 NEOWISE graced early morning skies, and transitioned to a fine dusk apparition for an encore performance in the last half of July.

F3 NEOWISE reminded us that all comets are worth keeping tabs on… just in case. But wait, there’s more. The Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) caught another intriguing object on August 2, 2020 as part of its extended sky survey mission: Comet C/2020 P1 NEOWISE is set to become a fine binocular object in late October and early November.

October 12, 2020October 16, 2020 by Paul M. Sutter

How to See What’s on the Other Side of a Wormhole Without Actually Traveling Through it

Wormholes are incredibly fascinating objects, but also completely hypothetical. We simply don’t know if they can truly exist in our universe. But new theoretical insights are showing how we may be able to detect a wormhole – from a spray of high-energy particles emitted at the moment of its formation.

October 12, 2020October 12, 2020 by Brian Koberlein

Black Holes Make Complex Gravitational-Wave Chirps as They Merge

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

Gravitational waves are produced by all moving masses, from the Earth’s wobble around the Sun to your motion as you go about your daily life. But at the moment, those gravitational waves are too small to be observed. Gravitational observatories such as LIGO and VIRGO can only see the strong gravitational waves produced by merging stellar-mass black holes.