Category Archives: Astronomy News

Solar storm hurls a CME toward Earth

With the cloudy skies and a full moon, we aren’t likely to see aurora here in Montreal, but the video of the CME is interesting.

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Space Weather News for Sept. 5, 2017
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A SOLAR STORM IS COMING: Yesterday, during a flurry of M-class solar flares, sunspot AR2673 hurled a CME toward Earth. NOAA forecasters say the cloud is likely to arrive late on Sept. 6th, causing moderately-strong (G2-class) geomagnetic storms with isolated periods of strong (G3-class) storming on Sept. 6th and 7th. Visit Spaceweather.com to view the aurora forecast and a movie of the CME leaving the sun.

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Above: The source of the incoming solar storm is huge sunspot AR2673, shown here in a Sept. 5th photo taken by amateur astronomer Philippe Tosi of Nîmes, France. An image of Earth was inserted for scale. More pictures of this sunspot may be found in the Space Weather Photo Gallery.

Possible Auroras this Thus and Fri

Space Weather News for August 30, 2017
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GEOMAGNETIC STORM IN THE OFFING: A canyon-shaped hole has opened in the sun’s atmosphere, and it is spewing a stream of high-speed solar wind toward Earth. NOAA forecasters say there is a 30% chance of polar geomagnetic storms (G1-class) when the gaseous material reaches our planet on August 31st. High-latitude sky watchers should be alert for auroras this Thursday and Friday. Visit Spaceweather.com for photos and updates.

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Above: This canyon-shaped “coronal hole” is a region in the sun’s atmosphere where the sun’s magnetic field has opened up, allowing solar wind to escape. Credit: NASA/SDO/Spaceweather.com

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Uranus and Neptune: Cloudy with a chance of diamonds

Researchers at SLAC National Accelerator Laboratory have recreated the ice giants’ diamond rain.

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Uranus and Neptune experience diamond rain deep within their atmospheres — and now scientists on Earth have watched this process occur in the lab. NASA/JPL-Caltech (Left, Uranus); NASA (Right, Neptune)
On Earth, we experience rain composed of liquid water. On Titan, it rains liquid methane. And on Uranus and Neptune, it rains solid diamonds. For the first time, researchers have now simulated and observed this process here on Earth, proving that this long-held assumption is likely correct, once and for all.

The work, published August 21 in Nature Astronomy, combined a high-powered optical laser with the X-ray free-electron laser at SLAC National Accelerator Laboratory, the Linac Coherent Light Source (LCLS). The LCLS creates X-ray pulses that last a million-billionths of a second, allowing for ultrafast high-precision monitoring of processes that occur all the way down to the scale of atoms. As a result, the researchers were able to watch tiny diamonds form as shock waves passed through plastic, offering a peek at processes that take place in planetary atmospheres on a much grander scale.

The experiment focused on inducing shock waves in a plastic material called polystyrene, which contains hydrogen and carbon — two elements found in abundance inside Uranus and Neptune. According to theory, methane (four hydrogen atoms and one carbon atom) inside the planets’ atmospheres forms hydrocarbon chains that in turn form diamonds in response to the right temperature and pressure. This occurs more than 5,000 miles (8,000 kilometers) beneath the planets’ surface. There, the diamonds precipitate out and sink deeper into the atmosphere, a “diamond rain.”

Though this has been assumed to be the case for decades, the exact process has never been observed in experiments on Earth before now. Some previous experiments failed because the pressures and temperatures inside the atmospheres of these planets cannot be created in the lab for long, and without the ability to record data at the speed afforded by the LCLS, any transitions were missed. Other experiments produced graphite or diamond, but were conducted at lower pressures or required the introduction of additional materials.

How long to travel to Alpha Centauri?

In April 2016, Russian high-tech billionaire Yuri Milner announced a new and ambitious initiative called Breakthrough Starshot, which intends to pour $100 million into proof-of-concept studies for an entirely new technology for star travel, aimed at unmanned space flight at 20% of light speed, with the goal of reaching the Alpha Centauri system – and, presumably, its newly discovered planet Proxima b – within 20 years. Is it possible?

I doubt it, but it’s an interesting read.  –cathypl
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80% chance of polar geomagnetic storms Friday

Space Weather News for August 3, 2017
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GEOMAGNETIC STORM WATCH: NOAA forecasters say there is an 80% chance of polar geomagnetic storms on Aug. 4th when a solar wind stream is expected to buffet Earth’s magnetic field. The wind is flowing from a canyon-shaped hole in the sun’s atmosphere, so wide that it is almost bisecting the solar disk. Storm levels could reach G2-category (moderately strong) during the late hours of Aug. 4th, subsiding to G1-category (minor) on Aug. 5th. Visit Spaceweather.com for more information and updates.

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Above: A canyon-shaped coronal hole (CH) is spewing solar wind toward Earth. This extreme ultraviolet image was taken by NASA’s Solar Dynamics Observatory.

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Source of Mars Trojans Might Be Mars Itself

Source of Mars Trojans Might Be Mars Itself

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A new study proposes a source for the mysterious Mars Trojans: Mars itself.

Mars Trojan

An artist’s conception of a Mars Trojan, ejected from the Red Planet.
Polishook / Weizmann Institute of Science

It’s one of the major mysteries of the inner solar system: How did Mars — a tiny world only a tenth the mass of Earth — capture its cluster of orbit-sharing Trojan asteroids?

Trojans are asteroids that co-orbit either ahead of a planet, at the L4Lagrangian point, or behind it at the L5 point. These regions are stable because the gravitational pull of the planet balances that of the Sun. Trojan asteroids have been discovered around Jupiter, Uranus, Neptune, Venus, and Mars. (Only one Trojan (2010 TK7) has been discovered related to the Earth, though the Osiris-REX mission bound for 101955 Bennu is currently on the hunt for more.)

Many studies have suggested that the asteroid belt, which lies just outside the orbit of Mars, may have been the source of the Mars Trojans. Now, a study published in the July 17th Nature Astronomy points to a new possible source: Mars itself.

NASA IRTF

NASA’s Infrared Telescope Facility
NASA

The study used observations from NASA’s Infrared Telescope Facility, based at the Mauna Kea Observatory in Hawai’i, to look at the spectra of two Mars Trojans: 311999 (initially desgnated 2007 NS2) and 385250 (2001 DH47. The light reflected off these asteroids shows a characteristic broad absorption band around 1 micron, consistent with the presence of olivine — a mineral rare in asteroids but common in the crust of Mars.

“Asteroids like this are very rare in the main belt of asteroids (0.4%),” says David Polishook (Weizmann Institute of Science, Israel). “Therefore, the chances that the few asteroids captured by Mars are olivine-rich asteroids is extremely low.” But Martian rovers and orbiters, and even Martian meteorites recovered on Earth, have shown that Mars itself offers an ample supply of olivine.

READ MORE

A spectacular CME is heading for Mars

A spectacular CME is heading for Mars, will the Martians see Aurora?

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Space Weather News for July 23, 2017
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MASSIVE EXPLOSION ON THE FARSIDE OF THE SUN: On July 23rd, NASA and European spacecraft observed a massive explosion on the far side of the sun. A spectacular CME tore through the sun’s atmosphere and it now appears to be en route to Mars. Earth will not feel the effects of the blast because of its location on the opposite side of the sun. However, the source of the eruption, old sunspot AR2665, will turn back toward our planet in early August, possibly bringing a new round of geomagnetic storms and auroras. Read all about it on today’s edition of Spaceweather.com.

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Above: This CME, blown into space by old sunspot AR2665 on July 23rd, appears to be en route to the planet Mars. Image credit: Solar and Heliospheric Observatory (SOHO)

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CME SWEEPS ASIDE COSMIC RAYS

Space Weather News for July 21, 2017
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CME SWEEPS ASIDE COSMIC RAYS: On July 16th, a CME hit Earth’s magnetic field, sparking two days of geomagnetic storms and beautiful auroras. The solar storm cloud also swept aside some of the cosmic rays currently surrounding our planet. A sudden decrease in deep space radiation was detected by a global network of neutron monitors as well as a space weather balloon in the stratosphere over California. Almost a week later, cosmic rays are finally returning to normal. Learn more about this event on today’s edition of Spaceweather.com.

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Above: This CME, blown into space by sunspot AR2665 on July 14th, reached Earth two days later and blew away many of the cosmic rays surrounding our planet. Image credit: Solar and Heliospheric Observatory (SOHO)

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gorgeous pictures of Jupiter’s Red Spot

For gorgeous pictures of Jupiter’s Red Spot, go to

https://www.missionjuno.swri.edu/news/juno-spots-great-red-spot

Here’s a sample! Got to site to see the full resolution images.
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This enhanced-color image of Jupiter’s Great Red Spot was created by citizen scientist Kevin Gill using data from the JunoCam imager on NASA’s Juno spacecraft.

The image was taken on July 10, 2017 at 07:07 p.m. PDT (10:07 p.m. EDT), as the Juno spacecraft performed its 7th close flyby of Jupiter. At the time the image was taken, the spacecraft was about 6,130 miles (9,866 kilometers) from the tops of the clouds of the planet.

Potential for Aurora Display!

Space Weather News for July 14, 2017
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STRONG SOLAR FLARE AND CME: After days of suspenseful quiet, huge sunspot AR2665 finally erupted on July 14th (0209 UT), producing a powerful M2-class solar flare. The explosion was underway for more than two hours and hurled a bright coronal mass ejection (CME) toward Earth. Geomagnetic storms and high-latitude auroras are likely when the CME arrives this weekend. Visit Spaceweather.com for images and updates.

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Above: The July 14th solar flare, recorded by extreme ultraviolet telescopes on board NASA’s Solar Dynamics Obse

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