What Caused the Recent Explosion at Jupiter?

An impact on Jupiter captured about 6:35 am on Sept. 10, 2012 from Dallas, Texas USA. Credit: George Hall.

A bright flash was spotted on Jupiter early on the morning of September 10, 2012, and astronomers were hoping to later see an impact “scar” which would provide more information about the object that slammed into the giant gas planet. Was it a comet, asteroid or a smaller meteor? But alas, no impact scar or debris field showed up on Jupiter’s face and the nature of this explosion may remain a mystery.

“By performing spectroscopic measurement of the debris field we hope to be capable of determining the nature of the impactor,” SETI astronomer Franck Marchis told Universe Today via email. “Without debris field it is virtually impossible since the bolide burned in the upper atmosphere. One day we may be capable of recorded a spectrum of the meteor itself (during the impact) but right now we don’t have such capabilities.”

The flash was first spotted by Dan Peterson, an amateur astronomer from Racine, Wisconsin who saw the flash as he was looking through a telescope, but he wasn’t recording his observations. He posted about his sighting on the Association of Lunar & Planetary Observers message board (ALPO), reporting the explosion, which occurred inside the southern edge of Jupiter’s northern equatorial belt of clouds.

Astrophotographer George Hall of Dallas, Texas happened to be shooting video of Jupiter at the time – although he wasn’t actually watching Jupiter himself. When he heard about Petersen’s visual, Hall reviewed his video and saw he had captured the flash at 6:35 a.m. CDT.

Video © George Hall. All rights reserved, used with permission.

Many astronomers were waiting for the next day when the impact region would be visible again to look for a debris field, as the explosion looked very similar to an impact that occurred in June 2010, which left an impact scar that was visible for several hours.

However, astronomer Mike Wong from the University of California, Berkeley had stayed up all night to estimate the amount of energy delivered by this fireball. As he posted on his blog, he predicted “that this event is too small to create a visible impact scar.”

He ended up being right.

Since there was no impact scar, the space telescopes like Hubble weren’t activated to take a look.

But some ground-based telescopes, like NASA’s Infrared Telescope Facility did take a look. Astronomer Glenn Orton, a senior research scientist at the Jet Propulsion Laboratory used the IRTF 3-meter telescope to look at Jupiter in the near-infrared, but came up empty in finding any debris or scar.

Observations of Jupiter taken with the IRTF telescope and the SpeX guide camera. The dark circle indicates the location of the flash observed on September 10 2012 (credit: G. Orton, Jet Propulsion Laboratory)

Orton was quoted in an article on ABC that he thinks a frozen comet may be the culprit.

“Most things in that part of the solar system are called Jupiter-family comets,” Orton said. “They’re ice balls that move in and have started co-orbiting around Jupiter.”

But Marchis said that since the object appears to have not entered the inner part of the planet atmosphere, the IR observation confirms that it was most likely a meteor.

And another scientist, Dr. Tony Phillips, an astronomer and the person behind Spaceweather.com, was interviewed on NPR’s Science Friday last week and he said the explosion was probably a small asteroid hitting Jupiter, but added, “We’ll probably never know for sure,”

But whatever it was, the event demonstrates how different astronomy is now from what it was just a few years ago.

“What is remarkable today is that amateur astronomers can detect such an event, and by using modern communication tools, the world of astronomers is instantaneously aware of it,” Marchis said. “Our solar system is full of those transient events (impact, volcanoes, storms), their early detection and monitoring is a great opportunity to characterize these planets or satellites, shining light on area of these bodies that cannot be seen when they are in their calm state.”

But there were a few dissenters, too. A small number of those posting on the astronomy community message boards said that since there wasn’t any scar visible, that the event really didn’t happen, and that Hall and Petersen were just seeing things. This may have been fueled by an initial discrepancy between Hall and Petersen’s timing report, but it was solved when Petersen found out that his clock was running 26 seconds fast. Others came up with different ideas about what it might have been, which included light from one of Jupiter’s moons, Adrastea, which was entering the eastern limb of Jupiter at about the same the time, to other, more wilder notions that might have involved alien spaceships.

But most astronomers concur the event did occur.

“Two observers reported the same event at almost the same time does not look to me that we could argue about the genuineness of the event,” Marchis said, noting that previous events like this have occurred in the past, with no impact scars. “Several events were observed in 1981 and 2010 as well and there were no scar as well. We can simply assume that the impactor was too small to reach the inner part of Jupiter atmosphere. It burned before reaching the lower deck because it was relatively small.”

Phillips mentioned that years ago, astronomers were skeptical that impacts like this happened in the Solar System today, but that all changed when Comet Shoemaker-Levy 9 impacted Jupiter in 1994, and with hundreds of telescopes watching the event, including the Hubble Space Telescope, “we got to see what a comet impact looked like, and analyze the chemical signature,” Phillips said.

But in this case, astronomers will very likely never know what caused the flash on Jupiter on September 10, 2012. But don’t worry – this won’t be the last time something like this happens. Marchis said in a comment on his blog that based on the current observations, it’s estimated that 50 meteors like this — or ones even more energetic — could be seen on Jupiter per year. We just don’t happen to catch very many of them in the act of occurring.

And if you’re excited about seeing explosions on other worlds, Jupiter isn’t the only place this happens. All our planets and moons get smacked occasionally, as the impact craters on the rocky bodies can attest. The best place to see this happening might be our own Moon. If you have a big enough telescope, you can join a group run through the Marshall Space Flight Center that has been watching the dark terrain of the Moon. They have observed over 260 explosions in the past 7 years.

Marchis said a better organized network of amateur astronomers watching Jupiter is important.

“I think it is important to organize a network of small telescopes that will monitor continuously Jupiter over a long period of time to be capable of estimating the flux of meteors in the outer part of the solar system, helping us to better estimate the age of icy satellite surface of Jupiter but also Saturn,” he said via email. “This is something we could do by combining professional and amateur astronomer efforts.”

Look for future updates as astronomers are trying to organize such a network.

Astrophoto: Crescent Moon Crossing

Astrophotographer Ken Lord caught an airplane crossing in front of a setting crescent Moon in British Columbia, Canada. Credit: Ken Lord

The things you can see out your door! On a previous image in this sequence, Ken Lord from British Columbia, Canada said he stuck his head out the door and happened to see a great view of the setting crescent Moon, so he ran and got his camera, took a few shots, and then managed to capture an airplane crossing directly in front of the beautiful crescent. Ken notes the mountains on the horizon are on Vancouver Island.

He used a Canon T1i, 170mm, 0.8 second exposure, ISO3200, F5.6. See more of Ken’s images at his Flickr page.

Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

Saturn Shows Off Its Shadow

Take a look up at the enormous shadow cast by Saturn onto its own rings in this raw image, acquired by NASA’s Cassini spacecraft on September 18, 2012.

Cassini captured this image from below Saturn’s ring plane at a distance of 1,393,386 miles (2,242,437 kilometers). It shows not only the gas giant’s shadow but also the wispy nature of the rings, which, although complex, extensive and highly reflective (the light seen on Saturn above is reflected light from the rings!) they are still very thin — less than a mile (about 1 km) on average and in some places as little as thirty feet (10 meters) thick.

Seen in the right light, some of the thin innermost rings can seem to nearly disappear entirely — especially when backlit by Saturn itself.

Views like the one above are once again possible because of Cassini’s new orbit, which takes it high above and below the ring plane, providing a new perspective for studying Saturn and its moons. Ultimately by next April the spacecraft will be orbiting Saturn at an inclination of about 62 degrees — that’d be like an orbit around Earth that goes from Alaska to the northernmost tip of Antarctica. (Find out how Cassini alters its orbit here.)

With this viewpoint Cassini will get some great views of Saturn’s north and south poles, which are gradually moving into their summer and winter seasons, respectively, during the ringed planet’s 29.5-Earth-year orbital period.

After more than 8 years in orbit Cassini is still fascinating us with enthralling images of Saturn on a regular basis. Read more about the Cassini mission here.

Cassini spots shepherd moons Pan (within the Encke Gap) and Prometheus (along the inner edge of the F ring) in an image acquired on Sept. 18, 2012

Images: NASA/JPL/Space Science Institute.

Shuttle Endeavour Lands for the Final Time at Edwards Air Force Base

En route to its final home in Los Angeles, space shuttle Endeavour is taking a victory tour of sorts through the southern part of the US. Yesterday, the shuttle took off from Kennedy Space Center, mounted atop the Shuttle Carrier Aircraft (SCA), and landed in Ellington Field near Johnson Space Center in Houston, flying over the Houston area to allow crowds of people to see the unusual spectacle of the shuttle and the 747 aircraft flying together low over the city. Today, the duo made a flyover of Tucson, Arizona, a request of space shuttle commander Mark Kelly so that his wife and former senator Gabrielle Giffords could watch — along with thousands of others in the Tucson area.

@ShuttleCDRKelly posted this picture on Twitter of himself and Gabrielle Giffords watching Endeavour fly over Tucson, Arizona.

Before flying over Houston, Endeavour and the SCA made low passes over NASA’s Stennis Space Center near Bay St. Louis, Mississippi, and Lockheed Martin’s Michoud Assembly Facility on the east side of New Orleans, where the shuttle’s external fuel tanks were built.

Following an overnight stay at Edwards Air Force Base on Thursday, the SCA and Endeavour will salute the surrounding area early Friday, Sept. 21 with a low flyby northbound to Sacramento and the San Francisco Bay area. Then, the aircraft will travel south, making a pass over NASA’s Ames Research Center, Vandenberg Air Force Base and NASA’s Jet Propulsion Laboratory before heading into the Los Angeles area.

Finally, the SCA and Endeavour will land about noon PDT at Los Angeles International Airport, for an arrival ceremony before Endeavour is taken off the SCA and transported to its permanent home at the California Science Center next month.

There is a “Spot The Shuttle” page on NASA’s Flickr stream where people have been uploading their images of the shuttle flying over, so check them out here.

This video shows excited students and faculty at the University of Arizona watching the shuttle fly over campus:

Next SpaceX Launch to ISS Set for October 7

SpaceX’s Falcon 9 rocket with a Dragon spacecraft is rolled out to the company’s launch pad in Cape Canaveral, Florida.
Credit: SpaceX

There will be more Dragons in space! The SpaceX Dragon’s next launch to the International Space Station has been scheduled for Sunday, October 7, 2012, NASA and SpaceX announced today. This will be the first of 12 contracted flights by SpaceX to resupply the space station and marks the second trip by a Dragon to the station, following a successful demonstration mission in May.

NASA said they have confirmed the status and readiness of the Falcon 9 rocket and its Dragon cargo spacecraft for the SpaceX CRS-1 mission, as well as the space station’s readiness to receive Dragon.

Dragon will be filled with about 450 kg (1,000 pounds) of supplies. This includes materials to support the 166 investigations planned for the station’s Expedition 33 crew, including 63 new science investigations. The Dragon will return about 330 kg (734 lbs) of scientific materials, including results from human research, biotechnology, materials and educational experiments, as well as about 230 kg (504 lbs) of space station hardware.

Materials being launched on Dragon will support experiments in plant cell biology, human biotechnology and various materials technology demonstrations, among others. One experiment, called Micro 6, will examine the effects of microgravity on the opportunistic yeast Candida albicans, which is present on all humans. Another experiment, called Resist Tubule, will evaluate how microgravity affects the growth of cell walls in a plant called Arabidopsis. About 50 percent of the energy expended by terrestrial-bound plants is dedicated to structural support to overcome gravity. Understanding how the genes that control this energy expenditure operate in microgravity could have implications for future genetically modified plants and food supply. Both Micro 6 and Resist Tubule will return with the Dragon at the end of its mission.

Expedition 33 Commander Sunita Williams of NASA and Aki Hoshide of the Japan Aerospace Exploration Agency will use the CanadArm2 to grapple the Dragon following its rendezvous with the station on Wednesday, Oct. 10. They will attach the Dragon to the Earth-facing port of the station’s Harmony module for a few weeks while crew members unload cargo and load experiment samples for return to Earth.

Dragon is scheduled to return in late October, and splash down via parachute in the Pacific Ocean off the coast of southern California.

Endeavour Departs Kennedy Forever for California Home

Image caption: Endeavour departs Kennedy Space Center forever on Sept 19 on last flight of NASA’s Space Shuttle Program. Credit: Ken Kremer

Under cloudy skies at first light, Space Shuttle Endeavour departed NASA’s Kennedy Space Center in Florida early Wednesday morning, Sept. 19, at about 7:22 a.m. EDT marking the final flight of NASA’s storied shuttle program.

The 100 ton Endeavour was secured atop NASA’s specially modified 747 Shuttle Carrier Aircraft for the cross-country ferry flight to California and Los Angeles International Airport.

The farewell flight went off without a hitch following two days of weather related delays. The shuttle & 747 Shuttle Carrier Aircraft (SCA) Jumbo Jet were in tip top shape.

Image caption: Endeavour’s Final Takeoff atop modified Boeing 747 from the Kennedy Space Center on Sept. 19 to California home. Credit: Ken Kremer – www.kenkremer.com

Hordes of local spectators and excited tourists from several continents caught a magnificent last glimpse of the piggybacked pair as they flew two looping north-south farewells over the Florida Space Coast making a low pass over nearby beaches, Patrick Air Force Base, Cape Canaveral Air Force Station, Kennedy Space Center Visitor Complex, and the shuttle landing runway at Kennedy before leaving the area to a mix of emotions both happy and sad.

Then all of a sudden after some 25 minutes, the dynamic duo disappeared without warning into the hazy clouds, flying on a north east heading and across the Florida panhandle.

After making low-level passes over NASA’s Stennis Space Center in southwest Mississippi and the Michoud Assembly Facility in New Orleans, Endeavour touched down at the Johnson Space Center at about 10:40 a.m. at Houston’s Ellington Field for a curtailed overnight stay.

Image caption: Endeavour departs Kennedy Space Center on Sept 19 on last flight accompanied by T-38 training jet. Credit: Ken Kremer

21 years after rolling out from the Palmdale assembly facility in California where she was constructed, Endeavour landed at Edwards Air Force Base at 3:50 p.m. EDT today, Sept. 20.

Early Friday morning (Sept. 21), Endeavour and the SCA will take flight on a victory lap initially heading north for low level passes over Sacramento and the San Francisco Bay area including the Golden Gate bridge – akin to the April 2012 flight of Enterprise over NYC. Then the pair will turn south and pass over NASA’s Ames Research Center, Vandenberg Air Force Base and NASA’s Jet Propulsion Laboratory before heading into the Los Angeles area and landing at Los Angeles International Airport.

In October, Endeavour will be towed over 2 days through the streets of Inglewood and Los Angelos to begin a new mission inspiring future explorers at her permanent new home at the California Science Center.

Endeavour was NASA’s youngest orbiter and flew 25 missions and traveled 122,883,151 miles during 299 days in space.

NASA’s trio of shuttle orbiters were forcibly retired in July 2011 following the successful STS-135 mission to the International Space Station.

Ken Kremer

Image caption: Endeavour prepares for final takeoff from the Shuttle Landing Facility at KSC. Credit: Brent Houston

Image caption: STS-130 astronaut Kay Hire greets space enthusiasts at the shuttle landing strip during the flyaway of Endeavour. Credit: Klaus Krueger

Ken Kremer with Space Shuttle Endeavour and the 747 Shuttle Carrier Aircraft (SCA) at the Shuttle Landing Facility at the Kennedy Space Center for final flyaway departure in September 2012 reporting for Universe Today. Credit: Brent Houston

Dawn Finds Asteroid Vesta is Rich in Hydrogen

This map from NASA’s Dawn mission shows the global distribution of hydrogen on the surface of the giant asteroid Vesta. Credit: NASA/JPL-Caltech/UCLA/PSI/MPS/DLR/IDA

This map from NASA’s Dawn mission shows the global distribution of hydrogen on the surface of the giant asteroid Vesta. Credit: NASA/JPL-Caltech/UCLA/PSI/MPS/DLR/IDA

The giant asteroid Vesta appears to have a bellyful of hydrogen. Data from the Dawn spacecraft reveals hydrated minerals in a wide area around Vesta’s equator. While Dawn did not find actual water ice, there are signs of hydrated minerals such as hydroxyl in the giant asteroid’s chemistry and geology.

“The source of the hydrogen within Vesta’s surface appears to be hydrated minerals delivered by carbon-rich space rocks that collided with Vesta at speeds slow enough to preserve their volatile content,” said Thomas Prettyman, lead scientist for Dawn’s gamma ray and neutron detector (GRaND) from the Planetary Science Institute.


A pitted terrain – looking much like potholes – mark where the volatiles, perhaps both hydroxyl and water, released from hydrated minerals boiled off.

Hydroxyl has recently been found on the Moon in permanently shadowed craters at the lunar poles, and so the Dawn scientists thought there might be a chance that water ice may have hunkered down near the surface around the giant asteroid’s poles, as well. But unlike Earth’s Moon, however, Vesta has no permanently shadowed polar regions, and so the strongest signature for hydrogen actually came from regions near the equator. And there, water ice is not stable.

Two papers were published this week in the journal Science that are based on observations from the low-altitude mapping orbit of the Dawn mission, an orbit which averaged about 210 km (130 miles) above the surface. Dawn left Vesta earlier this month, and is now on its way to its second target, the dwarf planet Ceres.

In addition to the paper authored by Prettyman and his team, a complementary paper, led by Brett Denevi, a Dawn participating scientist based at the Johns Hopkins University Applied Physics Laboratory describes the presence of pitted terrain created by the release of the volatiles.

In some cases, other space rocks crashed into these deposits later at high speed. The heat from the collisions converted the hydrogen bound to the minerals into water, which evaporated. The holes that were left as the water escaped stretch as much as 0.6 miles (1 kilometer) across and go down as deep as 700 feet (200 meters). Seen in images from Dawn’s framing camera, this pitted terrain is best preserved in sections of Marcia crater.

A distinctive “pitted terrain” observed by NASA’s Dawn mission on Vesta has also been seen on Mars. Credit: NASA/JPL-Caltech/University of Arizona/MPS/DLR/IDA/JHUAPL

“The pits look just like features seen on Mars, but while water was common on Mars, it was totally unexpected on Vesta in these high abundances,” said Denevi. “These results provide evidence that not only were hydrated materials present, but they played an important role in shaping the asteroid’s geology and the surface we see today.”

GRaND’s data are the first direct measurements describing the elemental composition of Vesta’s surface. Dawn’s elemental investigation by the instrument determined the ratios of iron to oxygen and iron to silicon in the surface materials. The new findings solidly confirm the connection between Vesta and a class of meteorites found on Earth called the Howardite, Eucrite and Diogenite meteorites, which have the same ratios for these elements. In addition, more volatile-rich fragments of other objects have been identified in these meteorites, which supports the idea that the volatile-rich material was deposited on Vesta.

Source: JPL

Weekly Space Hangout – Sep. 20, 2012

Once again, it’s time for the Weekly Space Hangout – our round up of all the big space news stories that you should be aware of. This week we talked about the following interesting stories in space and astronomy:

Contributors: Nicole Gugliucci, Ian O’Neill, Jason Major, Amy Shira Teitel, Nancy Atkinson

Host: Fraser Cain

We record the Weekly Space Hangout every Thursday morning live at 10:00 am Pacific / 1:00 pm Eastern as a live Google+ Hangout.

If you want to make sure you never miss an episode, put it into your calendar. Click here to see our next event on Google+.

Gaia Mission Passes Vital Tests

Caption: Fully integrated Gaia payload module with nearly all of the multilayer insulation fabric installed. Credit: Astrium SAS

Earlier this month ESA’s Gaia mission passed vital tests to ensure it can withstand the extreme temperatures of space. This week in the Astrium cleanroom at Intespace in Toulouse, France, had it’s payload module integrated, ready for further testing before it finally launches next year. This is a good opportunity to get to know the nuts and bolts of this exciting mission that will survey a billion stars in the Milky Way and create a 3D map to reveal its composition, formation and evolution.

Gaia will be operating at a distance of 1.5 million km from Earth (at L2 Lagrangian point, which keeps pace with Earth as we orbit the Sun) and at a temperature of -110°C. It will monitor each of its target stars about 70 times over a five-year period, repeatedly measuring the positions, to an accuracy of 24 microarcseconds, of all objects down to magnitude 20 (about 400,000 times fainter than can be seen with the naked eye) This will provide detailed maps of each star’s motion, to reveal their origins and evolution, as well as the physical properties of each star, including luminosity, temperature, gravity and composition.

The service module houses the electronics for the science instruments and the spacecraft resources, such as thermal control, propulsion, communication, and attitude and orbit control. During the 19-day tests earlier this month, Gaia endured the thermal balance and thermal-vacuum cycle tests, held under vacuum conditions and subjected to a range of temperatures. Temperatures inside Gaia during the test period were recorded between -20°C and +70°C.

“The thermal tests went very well; all measurements were close to predictions and the spacecraft proved to be robust with stable behavior,” reports Gaia Project Manager Giuseppe Sarri.

For the next two months the same thermal tests will be carried out on Gaia’s payload module, which contains the scientific instruments. The module is covered in multilayer insulation fabric to protect the spacecraft’s optics and mirrors from the cold of space, called the ‘thermal tent.’

Gaia contains two optical telescopes that can precisely determine the location of stars and analyze their spectra. The largest mirror in each telescope is 1.45 m by 0.5 m. The Focal Plane Assembly features three different zones associated with the science instruments: Astro, the astrometric instrument that detects and pinpoints celestial objects; the Blue and Red Photometers (BP/RP), that determines stellar properties like temperature, mass, age, elemental composition; and the Radial-Velocity Spectrometer (RVS),that measures the velocity of celestial objects along the line of sight.

The focal plane array will also carry the largest digital camera ever built with, the most sensitive set of light detectors ever assembled for a space mission, using 106 CCDs with nearly 1 billion pixels covering an area of 2.8 square metres

After launch, Gaia will always point away from the Sun. L2 offers a stable thermal environment, a clear view of the Universe as the Sun, Earth and Moon are always outside the instruments’ fields of view, and a moderate radiation environment. However Gaia must still be shielded from the heat of the Sun by a giant shade to keep its instruments in permanent shadow. A ‘skirt’ will unfold consisting of a dozen separate panels. These will deploy to form a circular disc about 10 m across. This acts as both a sunshade, to keep the telescopes stable at below –100°C, and its surface will be partially covered with solar panels to generate electricity.

Once testing is completed the payload module will be mated to the service module at the beginning of next year and Gaia will be launched from Europe’s Spaceport in French Guiana at the end of 2013.

Find out more about the mission here

The Universe Shines for Astronomy Photographer of the Year Winners

The overall winner in the Royal Observatory Greenwich’s annual Astronomy Photographer of the Year competition, M51 by Martin Pugh.

Want to see some absolutely gorgeous images of our Universe, all taken by amateur astrophotographers? Look no farther than the winners of the 4th annual Astronomy Photographer of the Year competition, held by the Royal Observatory Greenwich and Sky at Night Magazine. The winners were announced last night at the Royal Observatory, with a record number of entries received in 2012 from photographers from around the world.

“Many of the pictures have been taken with equipment that was out of the range of the amateur many years ago,” said Sir Patrick Moore, from the BBC’s Sky at Night, who is a judge in the competition. “I also like the choice of subjects: photographing people and the night skies is very difficult. The entrants have done very well indeed.”

The overall winner was from Australian Martin Pugh with his beautiful and crisp shot of M51, the Whirlpool Galaxy.

“The photographer has made the most of exceptionally good atmospheric conditions to capture an astonishing range of detail in his image of this iconic galaxy,” said Dr. Marek Kukula, the Royal Observatory Public Astronomer and a judge in the competition. “The beautiful spiral structure, dark lanes of dust, and the way the pink clouds of hydrogen really stand out – it’s a remarkable achievement by an amateur astronomer; one of the best images of M51 that I’ve seen.”

Here are more of the winning shots (and you can click on any of these images for the larger versions on Flickr or the ROG site):

The “People and Space” winner was Laurent Laveder from France, with “Facing Venus-Jupiter Close Conjunction.”

The “Our Solar System” category winner was Transit of Venus 2012 in Hydrogen-Alpha, by Chris Warren of the UK.

One of the year’s biggest astronomical events, the last transit of Venus for 105 years, was featured in numerous entries to the 2012 competition. The Our Solar System category was won by Chris Warren, for his fleeting image of the transit taken through a thin patch of cloud at Blackheath in London. F

Earth and Space category winner, “Orion, Taurus and the Pleiades” by Masahiro Miyasaka from Japan.

The winner of the Earth and Space category was Japan’s Masahiro Miyasaka for his image of Orion, Taurus and the Pleiades forming a dramatic backdrop above an eerie frozen landscape in Nagano.

“Young Astronomy Photographer of the Year” category winner was Jacob von Chorus from Canada

Young Astronomy Photographer of the Year accolade was won by 15 year old Jacob von Chorus from Canada, who impressed the judges with his beautiful shot of the Pleiades, showing many of the hot young stars which make up the cluster and the swirling wisps of blue-hued gas.

See more images of the winning and runner-up “Highly Commended” for each category at the ROG’s website.

See here for information about how you can participate in next year’s competition. Congrats to this year’s winners!