Category Archives: Astronomy News

Jupiter marks its closest opposition since 1963.

From Sky and Telescope:

Jupiter reaches opposition on September 26th just 591 million kilometers (367 million miles) from Earth, the closest they’ll pair for the year. Opposition distances vary depending on where the planet happens to be in its orbit when opposition comes around. The closer perihelion and opposition dates align, the closer the two planets will draw together and the brighter and larger the gas giant will shine.

Jupiter corona
Jupiter is so bright it creates an aureole in a bank of passing clouds earlier this month. Bob King

This go-round, Jupiter lines up with Earth just four months shy of its January 21, 2023, perihelion. It hasn’t been this close since the October 1963 opposition and won’t be again until October 7, 2129. That’s why it appears exceptionally large (49.9″ across) and bright (magnitude –2.9). But that’s only half the story.

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AURORAS ON JUPITER

Space Weather News for August 23, 2022
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AURORAS ON JUPITER: Yesterday, NASA released gorgeous new photos of auroras on Jupiter taken by the James Webb Space Telescope. Today’s edition of Spaceweather.com takes a deeper dive into the photos, explaining why Jupiter’s auroras are so much more than just oversized versions of our own. Spoiler alert: Volcanoes are involved. Full story @ Spaceweather.com.

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Above: Infrared auroras on Jupiter. Image credit: NASA/JWST

Surface Mass Ejection (SME) on Betelgeuse


Astronomers believe a chuck of matter ripped itself away from the surface of the star

Space Weather News for August 12, 2022
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WHAT JUST HAPPENED TO BETELGEUSE? Astronomers have identified a new type of stellar explosion: An SME or “Surface Mass Ejection.” Think of it as a CME on steroids; SMEs outmass CMEs by 400 billion to one. An SME on Betelgeuse may be responsible for the red supergiant’s recent dimming. Full story @ Spaceweather.com.

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Above: An artist’s concept of a Surface Mass Ejection (SME) on Betelgeuse.

Star discovered orbiting Milky Way’s supermassive black hole every 4 years

Star discovered orbiting Milky Way’s supermassive black hole every 4 years

The discovery should help astronomers better understand the extreme conditions at the center of our galaxy and what can survive there.
blackhole
SquareMotion/Shutterstock

Astronomers have discovered a star that orbits the supermassive black hole at the center of our galaxy every four years. That’s the shortest orbit ever observed around a supermassive black hole.

The newly discovered star, called S4716, is about four times more massive than our Sun and twice as hot. It survives extraordinary conditions, orbiting this black hole at a distance as close as 100 astronomical units, less than three times the distance of Pluto from the Sun.

The discovery should help astrophysicists better understand conditions near this gravitational behemoth at the center of the Milky Way and to better calculate its mass and radius.

READ MORE: https://astronomy.com/news/2022/07/star-discovered-orbiting-milky-ways-supermassive-black-hole-every-4-years

Micrometeoroid damage to James Webb Space Telescope imaged for first time

 The damage to NASA’s flagship observatory was significantly greater than pre-launch expectations.

JWSTillustration
Dotted Yeti/Shutterstock

The micrometeoroid that hit the James Webb Space Telescope in May caused significantly more damage than expected and will have a lasting impact on the telescope’s observations, according to a NASA report on the spacecraft’s performance. By contrast, other micrometeoroid impacts during the spacecraft’s first six months of operation have had a negligible effect.

The report contains an image showing the damage to one hexagonal segment of the observatory’s main mirror, called C3. “The single micrometeorite impact that occurred between 22—24 May 2022 exceeded prelaunch expectations of damage for a single micrometeoroid,” says the NASA report.

JWSTmirrordamage
Spot the difference: infrared images of the James Webb Space Telescope before launch (left) and after the micrometeoroid strike (right). The damaged C3 segment is to the bottom right of the mirror.
“Characterization of JWST science performance from commissioning” (July 12, 2022); NASA/ESA/CSA

The performance of the main mirror is determined by how much it deforms incoming starlight and measured by a quantity called wavefront error rms (root mean square). At the beginning the mission, the C3 segment had a wavefront error of 56 nanometers rms, a level similar to the main mirror’s other 17 segments. The impact increased C3’s wavefront error to 258 nm rms.

Spacecraft engineers can change the position and curvature of each segment and in this way were able to reduce the error to 178 nm rms. This has a measurable effect on the error of the main mirror as a whole. “However, the effect was small at the full telescope level because only a small portion of the telescope area was affected,” says the report.

The JWST team say the impact increased the error associated with entire main mirror to about 59 nm rms. “About 5-10 nm rms above the previous best wavefront error rms values.” That’s well within the performance limits the team were hoping for.

Nevertheless, the impact raises questions about the nature of the space environment where the JWST operates. This is a point in space about a million kilometers from Earth where the gravitational fields of the Sun, Moon and Earth are in balance and so provide a relatively stable location.

READ MORE https://astronomy.com/news/2022/07/micrometeoroid-damage-to-james-webb-space-telescope-imaged-for-first-time?

How artificial intelligence is changing astronomy

 How artificial intelligence is changing astronomy

Machine learning has become an essential piece of astronomers’ toolkits.
An android cups its hand over one ear of a pair of premium headphones, looking at a screen of data from a radio telescope in the background under a starry night sky

When most people picture an astronomer, they think of a lone person sitting on top of a mountain, peering into a massive telescope. Of course, that image is out of date: Digital cameras have long since done away with the need to actually look though a telescope.

But now the face of astronomy is changing again. With the advent of more powerful computers and sky surveys that generate unimaginable quantities of data, artificial intelligence is the go-to tool for the keen researcher of space. But where is all of this data coming from? And how can computers help us learn about the universe?

AI’s appetite for data

Chances are you’ve heard the terms “artificial intelligence” and “machine learning” thrown around recently, and while they are often used together, they actually refer to different things. Artificial intelligence (AI) is a term used to describe any kind of computational behavior that mimics the way humans think and perform tasks. Machine learning (ML) is a little more specific: It’s a family of technologies that learn to make predictions and decisions based on vast quantities of historical data. Crucially, ML creates models which exhibit behavior that is not pre-programmed, but learned from the data used to train it.

The facial recognition in your smartphone, the spam filter in your emails, and the ability of digital assistants like Siri or Alexa to understand speech are all examples of machine learning being used in the real world. Many of these technologies are now being used by astronomers to investigate the mysteries of space and time. Astronomy and machine learning are a match made in the heavens, because if there’s one thing astronomers have too much of — and ML models can’t get enough of — it’s data.

We’re all familiar with megabytes (MB), gigabytes (GB), and terabytes (TB), but data at that scale is old news in astronomy. These days, we’re interested in petabytes (PB). A petabyte is about one thousand TB, a million GB, or a billion MB. It would take around 10 PB of storage to hold every single feature-length movie ever made in 4K resolution — and it would take over a hundred years to watch them all.

READ MOREhttps://astronomy.com/news/2022/07/how-artificial-intelligence-is-changing-astronomy

Video of yesterday’s CME

Space Weather News for June 13, 2022
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MAGNIFICENT CME: Earlier today, an unusually slow solar flare hurled a magnificent CME into space. The explosion and its afterglow lasted nearly 8 hours. The CME could sideswipe Earth’s magnetosphere later this week, producing minor geomagnetic storms. Full story @ Spaceweather.com.

Don’t miss the next solar flare: Subscribers to our Space Weather Alert Service receive instant text messages when strong solar flares are underway.
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Above: Visit Spaceweather.com to watch a movie of today’s CME

 

METEOR OUTBURST POSSIBLE MAY 31

Space Weather News for May 24, 2022
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METEOR OUTBURST POSSIBLE NEXT WEEK: Debris from a shattered comet is approaching Earth, and it could cause a meteor outburst on May 31st. Experts caution that this is an uncertain forecast. The shower could be a great storm, a complete dud, or almost anything in between. Whatever happens, sky watchers in North America will be in the right place to see it; the shower is expected to peak almost directly above southern California. Sky maps and more @ Spaceweather.com.

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Above: Broken Comet 7P/Schwassmann-Wachmann 3, the source of next week’s possible meteor outburst.

 

A CME might be heading our way

Space Weather News for May 10, 2022
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X-CLASS SOLAR FLARE: An unusually-magnetized sunspot exploded on May 10th, producing an intense X1.5-class solar flare. Shortwave radio signals were blacked out around the Atlantic Ocean for as much as an hour, and now there’s a chance a CME is heading our way. Updates @ Spaceweather.com.

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Above: The extreme ultraviolet flash from today’s X-class solar flare. Credit: NASA’s Solar Dynamics Observatory

Blood Moon: Lunar Eclipse Sunday!

Lunar Eclipse Sunday!

 From CTV:

The best views will be in Ontario, Quebec and Atlantic Canada, where the moon will be already above the horizon by the time the eclipse is set to begin.

Click here to read full article, including how to view the eclipse if the sky is clouded over. 

From Astronomy Magazine:

Late on May 15, observers across the U.S. will be greeted with a total eclipse of the Moon, the first of two this year (the second one occurs early on the morning of Nov. 8). The Full Moon is two days from perigee, spanning nearly 33′ as it crosses the central part of Earth’s shadow, resulting in a longer-than-average 85-minute period of totality. The eclipse occurs with the Moon located in Libra the Balance; the later evening hours reveal the orange glow of Antares in neighboring Scorpius, providing a lovely complement to the orange-hued eclipsed Moon.

The visibility of the eclipse is time zone dependent. East Coast observers will see the whole eclipse in a dark sky. In the Midwest, the Full Moon rises in the eastern sky with the penumbral stages underway, enhancing the effect of the subtly progressing shadow. Observers in the Mountain time zone see the partial eclipse already underway in twilight. From the West Coast, the onset of totality occurs in twilight and the later stages of the eclipse are visible in a dark sky.

The lunar eclipse begins with the penumbral shadow — a subtle shading barely visible on the Moon’s lower limb — at 9:32 P.M. EDT. The Moon reaches the dark edge of the deep umbral shadow at 10:27 P.M. EDT. Dusky gray first creeps across the lunar surface and, as more of the Moon sinks into the shadow, an orange coloring will become noticeable, particularly through a telescope.