Solar System Antiquities Abound in Saturn’s Rings

The Cassini spacecraft observes three of Saturn's moons set against the darkened night side of the planet. Credit: NASA/JPL/Space Science Institute

Anyone looking for miscellanies from the early days of the Solar System can likely find them all in one place: the Saturn system. A new analysis of data from the Cassini spacecraft suggests that Saturn’s moons and rings are “antiquities” from around the time of our Solar System’s very beginnings.

“Studying the Saturnian system helps us understand the chemical and physical evolution of our entire solar system,” said Cassini scientist Gianrico Filacchione, from Italy’s National Institute for Astrophysics. “We know now that understanding this evolution requires not just studying a single moon or ring, but piecing together the relationships intertwining these bodies.”

The rings, moons, moonlets, and other debris date back more than 4 billion years. They are from around the time that the planetary bodies in our neighborhood began to form out of the protoplanetary nebula, the cloud of material still orbiting the sun after its ignition as a star.

Data from Cassini’s visual and infrared mapping spectrometer (VIMS) have revealed how water ice and also colors — which are the signs of non-water and organic materials –are distributed throughout the Saturnian system. The spectrometer’s data in the visible part of the light spectrum show that coloring on the rings and moons generally is only skin-deep.

Using its infrared range, VIMS also detected abundant water ice – too much to have been deposited by comets or other recent means. So the authors deduce that the water ices must have formed around the time of the birth of the solar system, because Saturn orbits the sun beyond the so-called “snow line.” Out beyond the snow line, in the outer solar system where Saturn resides, the environment is conducive to preserving water ice, like a deep freezer. Inside the solar system’s “snow line,” the environment is much closer to the sun’s warm glow, and ices and other volatiles dissipate more easily.

The effects of the small moon Prometheus loom large on two of Saturn's rings in this image taken a short time before Saturn's August 2009 equinox. Credit: NASA
The effects of the small moon Prometheus loom large on two of Saturn’s rings in this image taken a short time before Saturn’s August 2009 equinox. Credit: NASA

The colored patina on the ring particles and moons roughly corresponds to their location in the Saturn system. For Saturn’s inner ring particles and moons, water-ice spray from the geyser moon Enceladus has a whitewashing effect.

Farther out, the scientists found that the surfaces of Saturn’s moons generally were redder the farther they orbited from Saturn. Phoebe, one of Saturn’s outer moons and an object thought to originate in the far-off Kuiper Belt, seems to be shedding reddish dust that eventually rouges the surface of nearby moons, such as Hyperion and Iapetus.

A rain of meteoroids from outside the system appears to have turned some parts of the main ring system – notably the part of the main rings known as the B ring — a subtle reddish hue. Scientists think the reddish color could be oxidized iron — rust — or polycyclic aromatic hydrocarbons, which could be progenitors of more complex organic molecules.

One of the big surprises from this research was the similar reddish coloring of the potato-shaped moon Prometheus and nearby ring particles. Other moons in the area were more whitish.

“The similar reddish tint suggests that Prometheus is constructed from material in Saturn’s rings,” said co-author Bonnie Buratti, a VIMS team member based at NASA’s Jet Propulsion Laboratory, Pasadena, Calif. “Scientists had been wondering whether ring particles could have stuck together to form moons — since the dominant theory was that the rings basically came from satellites being broken up. The coloring gives us some solid proof that it can work the other way around, too.”

“Observing the rings and moons with Cassini gives us an amazing bird’s-eye view of the intricate processes at work in the Saturn system, and perhaps in the evolution of planetary systems as well,” said Linda Spilker, Cassini project scientist, based at JPL. “What an object looks like and how it evolves depends a lot on location, location, location.”

Filacchione’s paper has been published in the Astrophysical Journal.

Source: JPL

Astrophoto: Beautiful New Look at the Orion Nebula

M 42 in Orion using the 'Hubble "Palette.' Images by Gary Gonnella, image editing by Paul M. Hutchinson.

The enormous cloud of dust and gas that makes up the Orion Nebula is featured in this beautiful astrophoto. This image was a joint effort, with images taken by Gary Gonnella – a regular on our Virtual Star Parties – and image editing by Paul Hutchinson. Paul used the “Hubble Palette” – named for the Hubble Space Telescope and its capability of imaging in very narrow wavelengths of light using various filters. This enables astrophotographs to reveal details of objects in space that can’t be seen by the human eye. Here, the filters used produced different colors: were Hydrogen Alpha=Green, S=Red, O=Blue. Paul said he combined two exposures, a 1 minute and 10 second exposure, to reduce the blow-out in the bright center of the nebula. The results are striking!

Compare this great image to another image of the Orion Nebula, recently taken by the WISE telescope (Wide-field Infrared Survey Explorer), below. Colors in this image represents specific infrared wavelengths. Blue represents light emitted at 3.4-micron wavelengths and cyan (blue-green) represents 4.6 microns, both of which come mainly from hot stars. Relatively cooler objects, such as the dust of the nebulae, appear green and red. Green represents 12-micron light and red represents 22-micron light.

The Orion Nebula as seen by the WISE telescope. Image Credit: NASA/JPL-Caltech/UCLA
The Orion Nebula as seen by the WISE telescope. Image Credit: NASA/JPL-Caltech/UCLA

The Orion nebula is part of the larger Orion molecular cloud complex, which also includes the Flame nebula. This region is actively making new stars.

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.

New Crater Names Approved for Mercury’s South Pole & More

Mercury's southern polar region as seen from MESSENGER. (Credit: NASA/Johns Hopkins UniversityApplied Physics Laboratory/Carnegie Institution of Washington).

Move over, Tolkien & Tryggvadóttir. Yesterday, an announcement was made that the International Astronomical Union (IAU) approved proposed names for nine new craters on the planet Mercury. The names honor deceased writers, artists and musicians following the convention established by the IAU for naming features on the innermost world.

The announcement comes as NASA’s MESSENGER spacecraft has completed mapping of the surface of Mercury earlier this month. A good majority of these features were established at Mercury’s southern polar region, one of the last areas of the planet to be mapped by MESSENGER.

The craters honored with a newly assigned moniker are:

Donelaitis, named after 18th century Lithuanian poet Kristijonas Donelaitis, author of The Seasons and other tales and fables.

Petofi, named after 19th century Hungarian poet Sandor Petofi, who wrote Nemzeti dal which inspired the Hungarian Revolution of 1848.

Roerich, named after early 20th century Russian philosopher and artist Nicholas Roerich, who created the Roerich Pact of 1935 which asserted the neutrality of scientific, cultural and educational institutions during time of war.

Hurley, named after the 20th century Australian photographer James Francis Hurley, who traveled to Antarctica and served with Australian forces in both World Wars.

Lovecraft, named after 20th century American author H.P. Lovecraft, a pioneer in horror, fantasy and science fiction.

Alver, named after 20th century Estonian author Betti Alver who wrote the 1927 novel Mistress in the Wind.

Flaiano, named after 20th century Italian novelist and screenwriter Ennio Flaiano who was a pioneer Italian cinema and contemporary of Federico Fellini.

Pahinui, named after mid-20th century Hawaiian musician Charles Phillip Kahahawai Pahinui, influential slack-key guitar player and part of the “Hawaiian Renaissance” of island culture in the 1970’s.

L’Engle, named after American author Madeleine L’Engle, who wrote the young adult novels An Acceptable Time, A Swiftly Tilting Planet & A Wind in the Door. L’Engle passed away in 2007.

Five of the newly named craters in the south pole region of Mercury (circled in red). Note that the final portion of the USGS map, although recently released, has yet to be filled in! (Credit: USGS).
Five of the newly named craters in the south pole region of Mercury (circled in red). Note that the final portion of the USGS map, although recently released, has yet to be filled in! (Credit: USGS).

The nine new crater names join 95 others named thus far. The MESSENGER surface mapping campaign has been ongoing since the spacecraft’s first flyby of Mercury in January 2008. MESSENGER entered permanent orbit around world on March 18th, 2011.

MESSENGER missions operations engineer Ray Espiritu was instrumental in getting Pahinui’s name in the running.

“I wanted to honor the place where I grew up and still call home,” Espiritu said. ”The Pahinui crater contains a possible volcanic vent, and its name may inspire other scientists as they investigate the volcanic processes that helped to create Mercury, just as investigation of the Hawaiian volcanoes helps us understand the volcanic processes that shape Earth as we know it today.”

Pahinui Crater. (Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington).
Pahinui Crater. (Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington).

Lovecraft is another interesting selection on the list. The name of the famous horror writer was in the running last month for the naming of Pluto’s moons P4 & P5, and New Horizons principle investigator Alan Stern hinted that Lovecraft may still find a home on a surface feature as New Horizons reveals Pluto & Charon in July 2015. It would be a fitting tribute to a fine writer. Could we end up with Lovecraft marking not only the solar system’s “hubs of hell” on Mercury, but its frozen outer wastelands as well?

There was more news yesterday in the realm of astrogeology and the planet Mercury. The IAU Working Group for Planetary System Nomenclature also made the distinction between features described as valles and catenae on the surface of Mercury. Catenae are described as crater chains, and MESSENGER has sufficient resolution that several valles have been revealed as such. Catenae on Mercury are named after radio astronomy observatories, while valles are named after abandoned cities of antiquity. Thus, Haystack Vallis is now Haystack Catena, Goldstone Vallis is now Goldstone Catena, and Arecibo Vallis is now Arecibo Catena, and, well, you get the idea.

Arecibo  Catenae (formerly known as Arecibo Vallis) as imaged by MESSENGER in 2008. (Credit:  NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington).
Arecibo Catenae (formerly known as Arecibo Vallis) as imaged by MESSENGER in 2008. (Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington).

MESSENGER has proven to be a boon for planetary science. The spacecraft was launched in 2004 and took almost 7 years and 6 flyby assists (one past the Earth, two past Venus and three past Mercury) to become the first spacecraft to orbit the tiniest planet in our solar system. Mercury was first seen up close by Mariner 10 in 1974 and even then we only mapped 45% of its surface. Scientists had to wait until MESSENGER to fill in the remainder of Mercury’s map.

The next mission to Mercury isn’t until the planned arrival of the joint ESA/JAXA BepiColombo mission in 2022.

And don’t forget to watch for Mercury as it reaches greatest elongation on Easter Day low in the dawn sky. I managed to catch sight of it low to the east with binoculars for the first time this apparition this morning about 40 minutes prior to local sunrise. It’s amazing to think that ground-based professional telescopes & even amateur astronomers can actually image fuzzy details on the planet’s surface that match up with what MESSENGER is revealing!

All fascinating stuff to contemplate as  we welcome the newest named craters to our ever expanding map of Mercury… now, will there ever be a Miskatonic University within the walls of Lovecraft crater?

-Explore these recently named craters and more  using the USGS inactive Astrogeology Science Center.

-Also check out this animation of the south polar region of Mercury and more as imaged by MESSENGER.

 

 

 

Chris Hadfield’s Top 5 Videos from Space

Chris Hadfield all dressed up for another day in space. Credit: Chris Hadfield (Twitter)

Chris Hadfield — the ever-tweeting, always charming Canadian running the space station these days — has had an eventful few months in space. If he’s not chatting with Captain Kirk, he’s playing guitar or, as it turns out, making very watchable videos.

Being on television requires a certain flair. You need to talk in sound bites, cultivate a charismatic presence, and keep the action moving enough so people don’t flip the channel. For an astronaut, who usually works methodically, carefully and slowly, working on television must be fully alien (pun intended) to how one does the technical parts of the job.

But Hadfield — who knows how to study a situation and make the most of it — has created videos with hundreds of thousands of views on YouTube. Whatever he’s doing is working.

Universe Today checked up on Hadfield’s secrets to success by watching the most popular videos in a playlist curated by the Canadian Space Agency. Here are the top five. Strangely, the last one doesn’t even include Hadfield’s face or voice.

5) Chris Hadfield Talks with the Queen’s Representative in Canada

If you’re all about cute questions from kids, or enjoy a brush with royalty, this lengthy press conference with Hadfield is very interesting. This is a bit of a marathon charm session on Hadfield’s part, but he pulls it off with his charismatic aplomb. One of the best answers demonstrates what he’s learned about weightless life: “I can fly. I can go in different directions,” Hadfield says enthusiastically, spinning before the camera.

4) Chris Hadfield Demonstrates How Astronauts Wash Their Hands in Zero G

For a question that came out of a routine Q&A with kids, Hadfield’s performance is pretty good. He demonstrates that soapy water looks like some sort of Teenage Mutant Ninja Turtles-like ooze in space, and compares life on the space station to life on a sailboat, all while simply washing his hands. It’s almost existential.

3) Nail Clipping in Space

It turns out that Hadfield chooses to cut his nails because long ones interfere with his guitar playing. We wouldn’t want that to happen (and neither would the Barenaked Ladies), so fortunately Hadfield gets right on the problem, positions himself over an air vent and trims them with an ordinary nail clipper. Charmingly, this was not fully scripted, as he makes a mistake with the first clipping.

2) Chris Hadfield’s Space Kitchen (aka how to make a peanut butter sandwich in space)

With words you’d never hear on Martha Stewart — “We’ve got one tortilla. Oh, got away!” — Hadfield slathers condiments on to a tortilla and eats it. His sense of humor helps break up a very routine act; we’d be scared to be one of his kids after seeing the stern way in which he says, “Disinfectant wipe!”

1) Mixed Nuts in Space

This video is oddly mesmerizing, and that’s not just because of the UFO-type music near the beginning. It’s quite a simple setup: Hadfield shoots a bunch of nuts floating around inside of a can. But face it, it looks awfully weird for those of us used to grabbing similar packages off the kitchen shelf. Maybe that’s why this video has more than 4 million views.

New Stars: Blazing and Blue

This image from the Wide Field Imager on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile. Credit: ESO

A new image from ESO shows a pretty sprinkling of bright blue stars, the star cluster NGC 2547, a group of recently formed stars in the southern constellation of Vela. Even though we recently got a more precise estimate on how old the Universe is from the Planck mission (13.82 billion years), this is a look at some fairly young — new and blue — stars.

But how young are these cosmic youngsters really? ESO scientists say that although the exact ages of these stars remain uncertain, estimates range from 20 to 35 million years old. That doesn’t sound all that young, after all. However, our Sun is 4.6 billion years old and has not yet reached middle age. That means that if you imagine that the Sun as a 40 year-old person, the bright stars in the picture are three-month-old babies.

Most stars do not form in isolation, but in rich clusters with sizes ranging from several tens to several thousands of stars. Clusters are key objects for astronomers studying how stars evolve through their lives. The members of a cluster were all born from the same material at about the same time, making it easier to determine the effects of other stellar properties.

While NGC 2547 contains many hot stars that glow bright blue, also visible are one or two yellow or red stars which have already evolved to become red giants. Open star clusters like this usually only have comparatively short lives, of the order of several hundred million years, before they disintegrate as their component stars drift apart.

This picture was created from images forming part of the Digitized Sky Survey 2. It shows the rich region of sky around the young open star cluster NGC 2547 in the southern constellation of Vela (The Sail). Credit:  ESO/Digitized Sky Survey 2. Acknowledgement: Davide De Martin
This picture was created from images forming part of the Digitized Sky Survey 2. It shows the rich region of sky around the young open star cluster NGC 2547 in the southern constellation of Vela (The Sail). Credit:
ESO/Digitized Sky Survey 2. Acknowledgement: Davide De Martin

The star cluster NGC 2547 lies in the southern constellation of Vela (The Sail), about 1500 light-years from Earth, and is bright enough to be easily seen using binoculars. It was discovered in 1751 by the French astronomer Nicolas-Louis de Lacaille during an astronomical expedition to the Cape of Good Hope in South Africa, using a tiny telescope of less than two centimeters aperture.

Between the bright stars in this picture you can see plenty of other objects, especially when zooming in. Many are fainter or more distant stars in the Milky Way, but some, appearing as fuzzy extended objects, are galaxies, located millions of light-years beyond the stars in the field of view.

Source: ESO

Book Review: Vistas of Many Worlds

Vistas of Many Worlds: A Journey Through Space and Time by Erik Anderson (Ashland Astronomy Studio)

While many astronomy books are based around images that show us how the Universe appears to us right now, as seen through the sensitive electronic eyes of powerful space telescopes and observatories around the world, Erik Anderson’s Vistas of Many Worlds: a Journey Through Space and Time takes a different, but no less fascinating, approach and shows us what the night sky used to look like, will one day look like, and how it may look from other much more distant worlds.

The nearby orange dwarf star Epsilon Eridani reveals its circumstellar debris disks in this close-up perspective. (Pages 14-15)
The nearby orange dwarf star Epsilon Eridani reveals its circumstellar
debris disks in this close-up perspective. (Pages 14-15)

Written and illustrated by Erik Anderson of the Ashland Astronomy Studio in Ashland, Oregon, Vistas of Many Worlds first takes us on a tour of our local region of the galaxy, introducing us to some of our Sun’s closest neighbors in space. From Alpha Centauri to Altair, we get scientifically-based renderings of several nearby stars as they’d appear close up, along with a detailed description of each — as well as an accurate depiction of the background stars (including the Sun) as they’d appear from such slightly different vantage points. We soon find out there’s an amazing amount of variety in our own stellar neighborhood alone!

Next we get a tour through time itself with images and detailed descriptions of the night sky as it appeared at various points in Earth’s history. Based on the actual movements of the stars across the galaxy, Anderson is able to accurately show the star-filled sky as it looked when the ocean cascaded over the Strait of Gibraltar to fill in the Mediterranean 5.3 million years ago, when the ancestors of modern humans were first learning to use fire 1.5 million years ago… and also what it will look like when the Solar System eventually dips back down into the galactic plane 25 million years from now — a time when nearly all the stars in the sky will be strangers, unfamiliar to us today.

After that Anderson takes us on a hunt for exoplanets, both known and imagined. We first visit the star systems that have been recently discovered to host planets — some a little like Earth, some a little like Jupiter, and some like nothing we’ve ever seen before. Then it’s off to look for truly Earthlike worlds by looking back at how our own planet became so favorable for life in the first place. From a stable parent star like the Sun to the chance birth of a large, stabilizing moon, from the delivery of life-sustaining liquid water (that stays liquid!) to having a protective “big brother” gas giant ready to take the heavy hits, and eventually what first drew organisms up from the sea onto dry land, Anderson speculates about Earth’s distant exoplanetary twins by reflecting on our planet itself.

The Earth's ancient past is depicted as it looked 4.4 million years ago when an ancient ape, "Ardi" the Ardipithecus, roamed Africa. (Pages 36-37)
The Earth’s ancient past is depicted as it looked 4.4 million years ago
when an ancient ape, “Ardi” the Ardipithecus, roamed Africa. (Pages 36-37)

And all the while showing what stars are where in the sky.

Vistas of Many Worlds is a true gem… it inspires imagination with the turn of each page. Anderson’s photorealistic computer-generated illustrations are lush and intriguing, and he does an excellent job combining speculation with scientific knowledge. It’s science as envisioned by an artist as well as art created by a scientist — truly the best of both many worlds.

The 123-page 9″ x 12″ hardcover book can be purchased on the Ashland Astronomy Studio’s website here, as well as on Amazon.com.

An iBook edition is soon to be announced.

A primordial ocean-world orbited by two moons is depicted in Ptolemy's Cluster (star cluster M7). The scene parallels Earth's own natural history, commemorating the origins of watery oceans out of volcanic steam and infalling comets. (Pages 96-97)
A primordial ocean-world orbited by two moons is depicted in Ptolemy’s
Cluster (star cluster M7). The scene parallels Earth’s own natural history,
commemorating the origins of watery oceans out of volcanic steam and
infalling comets. (Pages 96-97)

All images ©Erik Anderson/Ashland Astronomy Studio. All rights reserved. Used with permission.

Gallery: Dragon Splashes Down Successfully

Dragon is slowed by three main parachutes prior to splashdown into the Pacific Ocean. Credit: SpaceX.

Splashdown! The SpaceX Dragon has returned home safely, splashing down in the Pacific Ocean at 16:36 UTC (12:36 p.m. EDT) on Tuesday, March 26, 2013. “Recovery ship has secured Dragon,” Tweeted SpaceX CEO Elon Musk. “Powering down all secondary systems. Cargo looks A-OK.”

A team of SpaceX engineers, technicians and divers will recover the vehicle off the coast of Baja, California, for the journey back to shore, which NASA said will take 30-48 hours.

The big job will be unloading the 3,000- plus pounds (1,360 kg) of ISS cargo and packaging inside the spacecraft. The Dragon is currently the only vehicle capable of returning cargo and important scientific experiments back to Earth.

“The scientific research delivered and being returned by Dragon enables advances in every aspect of NASA’s diverse space station science portfolio, including human research, biology and physical sciences,” said Julie Robinson, International Space Station Program
scientist. “There are more than 200 active investigations underway aboard our orbiting laboratory in space. The scientific community has
eagerly awaited the return of today’s Dragon to see what new insights the returned samples and investigations it carries will unveil.”

See more images below of Dragon’s return and mission to the ISS; we’ll be adding more as the SpaceX team supplies them!

Here’s a gif image of the splashdown:

A series of images shows the Dragon splashdown. Credit: SpaceX.
A series of images shows the Dragon splashdown. Credit: SpaceX.
This picture captures the Dragon just as it hits the water in the Pacific Ocean. Credit: SpaceX.
This picture captures the Dragon just as it hits the water in the Pacific Ocean. Credit: SpaceX.
Dragon was released from the International Space Station on March 26, 2013 during the CRS-2 mission. Credit: SpaceX.
Dragon was released from the International Space Station on March 26, 2013 during the CRS-2 mission. Credit: SpaceX.

Dragon’s release from Canadarm2 occurred earlier today at 10:56 UTC. The Expedition 35 crew commanded the spacecraft to slowly depart from the International Space Station

Dragon attached to the International Space Station during the CRS-2 mission. Credit: NASA.
Dragon attached to the International Space Station during the CRS-2 mission. Credit: NASA.
Dragon in orbit during the CRS-2 mission. Credit: NASA/CSA/Chris Hadfield
Dragon in orbit during the CRS-2 mission. Credit: NASA/CSA/Chris Hadfield

Among the the scientific experiment returned on Dragon was the Coarsening in Solid-Liquid Mixtures (CSLM-3) experiment, which also launched to space aboard this Dragon. CLSM-3 studies how crystals known as dendrites form as a metal alloy becomes solid. The research could help engineers develop stronger materials for use in automobile, aircraft and spacecraft parts.

Dragon also is returning several human research samples that will help scientists continue to examine how the human body reacts to long-term spaceflight. The results will have implications for future space exploration and direct benefits here on Earth.

The mission was the second of at least 12 cargo resupply trips SpaceX plans to make to the space station through 2016 under NASA’s
Commercial Resupply Services contract.

New Kind of “Runt” Supernovae Could be Lurking Unseen

This artist's conception shows the suspected progenitor of a new kind of supernova called Type Iax. Material from a hot, blue helium star at right is funneling toward a carbon/oxygen white dwarf star at left, which is embedded in an accretion disk. In many cases the white dwarf survives the subsequent explosion. Credit: Christine Pulliam (CfA)

Imagine this “Death from the Skies” scenario; a tiny supernova lurks unseen near our Sun. Astronomers from the Harvard-Smithsonian Center for Astrophysics (CfA) announced the discovery of just such an object today and while it is not nearby, this new kind of supernova is so faint it has been hiding in the shadows.

Until now, supernovae have come in two main versions. In one scenario, a huge star, 10 to 100 times more massive as our Sun, collapses causing a colossal stellar explosion. Another scenario, known as Type Ia supernovae, occurs when material from a parent star streams onto the surface of a white dwarf. Over time, so much material falls onto the white dwarf that it raises the core temperature igniting carbon and causing a runaway fusion reaction. This event completely disrupts the white dwarf and results in a colossal stellar explosion.

Now astronomers have found a third type that is fainter and less energetic than a Type Ia. Called a Type Iax supernova, it is “essentially a mini supernova,” says lead author of the study Ryan Foley, Clay Fellow at the Harvard-Smithsonian Center for Astrophysics (CfA). “It’s the runt of the supernova litter.”

Being only about one-hundredth as bright as their supernova siblings, Foley calculates that Type Iax supernovae are about as third as common as Type Ia supernovae. The researchers also did not find them in elliptical galaxies, filled with older stars, suggesting that Type Iax supernovae come from young star systems.

So far, Foley and his team identified 25 examples of this new type of supernova. Based on observations, the team found that the new Type Iax supernovae come from binary star systems containing a white dwarf and a companion star that has burned all of its hydrogen, leaving an outer layer that is helium rich.

In a press release, Foley says they are not sure what triggers the Type Iax supernova. One explanation involves the ignition of the outer helium layer from the companion star. The resulting shockwave slams into the white dwarf and disrupts it, causing the explosion. Alternately, the white dwarf might ignite first due to the overlying helium shell it has collected from the companion star.

“Either way, it appears that in many cases the white dwarf survives the explosion unlike in a Type Ia supernova where the white dwarf is completely destroyed,” says Foley. “The star will be battered and bruised but it might live to see another day.”

Supernovae explosions release so much energy as heat and light that they outshine entire galaxies for brief periods of time. The extremely hot conditions naturally create new heavier elements, such as gold, lead, nickel, zinc and copper. The explosion enriches the surrounding area leaving material for new stars to form.

“Type Iax supernovas aren’t rare, they’re just faint,” explains Foley. “For more than a thousand years, humans have been observing supernovas. This whole time, this new class has been hiding in the shadows.”

This research has been accepted for publication in The Astrophysical Journal and is available online.

Carnival of Space #294

This week’s Carnival of Space is hosted by our pal Ray Sanders at his Dear Astronomer website!

Click here to read Carnival of Space #294.

And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, sign up to be a host. Send an email to the above address.

Win a Copy of “Your Ticket to the Universe”

Your Ticket to the Universe: A Guide to Exploring the Cosmos (Available April 2)

A beautiful new book, “Your Ticket to the Universe: A Guide to Exploring the Cosmos” highlights some of the most fascinating and important sites in the universe, from those closest to us in our Solar System all the way to the Milky Way galaxy and beyond. All of these celestial landmarks are illustrated with beautiful, vivid photographs that bring them to life. You can read Jason Major’s full review of this book here.

This is an awesome compilation of images and information, and the book was written by by Kimberly K. Arcand and Megan Watzke, media coordinator and press officer and for NASA’s Chandra X-ray Observatory.

Thanks to Smithsonian Books, Universe Today has five copies of this book to giveaway!

In order to be entered into the giveaway drawing, just put your email address into the box at the bottom of this post (where it says “Enter the Giveaway”) before Monday, April 1, 2013. We’ll send you a confirmation email, so you’ll need to click that to be entered into the drawing.

We’re only going to use these email addresses for Universe Today giveaways/contests and announcements. We won’t be using them for any other purpose, and we definitely won’t be selling the addresses to anyone else. Once you’re on the giveaway notification list, you’ll be able to unsubscribe any time you like.