Bridge Between the Stars – NGC 602: Hubble Visualization by Jukka Metsavainio

NGC 602 Parallel Hubble Visualization by Jukka Metsavainio

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It’s been awhile hasn’t it? Time may have passed, but absence makes the heart grow fonder. For those of you who have missed our very special dimensional looks into the Cosmos, then it’s high time we let our minds and eyes relax and we take a 200 thousand light-year distant journey towards the edge of the Small Magellanic Cloud for a look at a bright, young open cluster of stars known as NGC 602…

Whenever we present a dimensional visualization it is done in two fashions. The first is called “Parallel Vision” and it is much like a magic eye puzzle. When you open the full size image and your eyes are the correct distance from the screen, the images will seem to merge and create a 3D effect. However, for some folks, this doesn’t work well – so Jukka has also created the “Cross Version”, where you simply cross your eyes and the images will merge, creating a central image which appears 3D. Upon further study, we’ve also come to realize that there is a certain percentage of people who also are unable to make this happen as well. You aren’t weird – just a percentage. Here’s why…

Typical for hunting animals (as opposed to ‘prey’ animals), we have our eyes set in the front of our heads. Our eyes are typically about 2½ inches apart, and so they see slightly different versions of the scene in front of them, from which the visual part of our brain constructs an internal three-dimensional model. Thus a human being can directly estimate the distance of something without moving a muscle – an important evolutionary advantage for a hunter. The trick is to then ‘fool’ the brain into processing the photographic images as if they really were distant scenes, not just color photos a few inches away. First, you will need a piece of white card, about 12 inches long. You hold the card vertically between your eyes and the pictures, so that it touches the centerline of the stereo pairs. Next? A pair of cheap reading glasses. If you usually have to wear reading glasses then you’ll need a higher power. Try different pairs in the store until you find one that will allow you see sharply no further away than a little over 12 inches. That’s it! Then sit back, relax and prepare to be blown away…

NGC 602 Cross Hubble Visualization by Jukka Metsavainio
NGC 602 Cross Hubble Visualization by Jukka Metsavainio

Cruising along some 200 thousand light-years away from the Milky Way is the Small Magellanic Cloud – a satellite galaxy of ours. Sitting on its edge is cloud of gas and dust which comprise a nebula known as M90, and within it shines a sparkling cluster of new stars called NGC 602. But these new stars aren’t shy… They’re hot and massive. The radiation and shock waves which pour from them have pushed the nebula away, compressing it and triggering new star formation. While these pre-main sequence embryonic suns lay hidden to all but infrared wavelengths, the beauty of this area is the chemical properties it shares with our own galaxy.

According to the studies of L.R. Carlson (et al) NGC 602’s star formation at a low chemical abundance makes it a “good analog to the early universe in terms of examining the processes and patterns of star formation. This cluster in particular is ideally suited to this aim. Its location in the wing of the SMC means that, while its chemical properties should be similar to those of the rest of the galaxy, it is relatively isolated.” Isolated… But young, very young. Says Carlson, “This pre-Main Sequence population formed coevally with the central cluster about 5 million years ago. Spitzer Space Telescope (SST) images of the region in all four Infrared Array Camera (IRAC) bands reveal a second population of Young Stellar Objects (YSOs), which formed after the stars seen with HST/ACS imaging. Some of these very young objects are still embedded in nebular material. We infer that star formation started in this region less than five million years ago with the formation of the central cluster and gradually propagated towards the outskirts where we find evidence of on going star formation less than a million years old.”

Another interesting factor is NGC 602’s position in the wing of the Small Magellanic Cloud leading to the Magellanic Bridge – a stream of neutral hydrogen which connects the two Magellanic Clouds like a invisible cord. While it’s mostly comprised of low-metallicity gas there have been two early-type stars found inside it. The Magellanic Bridge is also a favored region for investigations of interstellar gas and star formation in very low metallicity region… Much like the home of our bright young cluster. Why is this so fascinating? Because studying star formation in regions like this gives astronomers a look at what may happen during galaxy formation – long before heavier elements are created from successive generations of stars undergoing nuclear fusion.

So, as you look deep into this bridge between the stars, gaze with wonder at the long “elephant trunks” of dust and turn your mind towards these beautiful, bright blue stars still forming from gravitationally collapsing gas clouds. It is a very unique event, occurring where it should not happen – but is. A true bridge between the stars…

And touchstone to the Cosmos.

Many thanks to Jukka Metsavainio for his magic with Hubble Space Telescope images and allowing us this incredible look inside another mystery of space.

Constraining the Orbits of Planet X and Nemesis

Artists impression of the hypothetical star, Nemesis (Wikipedia)

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If Planet X was out there, where would it be? This question posed by an Italian researcher turns out to be a lot more involved than you’d think. As opposed to all the 2012 idiocy hype flying around on the internet, this research is actually based on a little thing called science. By analysing the orbital precession of all the inner-Solar System planets, the researcher has been able to constrain the minimum distance a hypothetical object, from the mass of Mars to the mass of the Sun, could be located in the Solar System. As most of the astronomical community already knows, the two purveyors of doom (Planet X and the Sun’s evil twin, Nemesis) exist only in the over-active imaginations of a few misinformed individuals, not in reality…

Planet X and Nemesis are hypothetical objects with more grounding in ancient prophecy and doomsday theories based on pseudo-science. This might be the case, but Planet X came from far more rational beginnings.

The name “Planet X” was actually coined by Percival Lowell at the start of the 20th century when he predicted there might be a massive planet beyond the orbit of Neptune. Then, in 1930, Clyde Tombaugh appeared to confirm Lowell’s theory; a planet had been discovered and it was promptly named Pluto. However, as time went on, it slowly became apparent that Pluto wasn’t massive enough to explain the original observations of the perturbations of Uranus’ orbit (the reason for Lowell’s Planet X prediction in the first place). By the 1970’s and 80’s modern observation techniques proved that the original perturbations in Uranus’ orbit were measurement error and not being caused by a massive planetary body. The hunt for Planet X pretty much ended with the discovery of Pluto in 1930, but it never lived up to its promise as a massive planetary body (despite what the woefully erroneous doomsday theories say otherwise).

Now an Italian researcher has published results from a study that examines the orbital dynamics of the inner-Solar System planets, and relates them to the gravitational influence of a massive planetary body orbiting the Sun from afar.

To cut a long story short, if a massive planetary body or a small binary sibling of the Sun were close to us, we would notice their gravitational influence in the orbital dynamics of the planets. There may be some indirect indications that a small planetary body might be shaping the Kuiper Cliff, and that a binary partner of the Sun might be disturbing the Oort Cloud every 25 million years or so (relating to the cyclical mass extinctions in Earth’s history, possibly caused by comet impacts), but hard astronomical proof has yet to be found.

Lorenzo Iorio from the National Institute of Nuclear Physics in Pisa (Italy) has taken orbital data from many years of precise observations and used his computations to predict the closest possible distance at which a massive planet could orbit if it was out there.

It turns out that all the planets the mass of Mars and above have been discovered within the Solar System. Iorio computes that the minimum possible distances at which a Mars-mass, Earth-mass, Jupiter-mass and Sun-mass object can orbit around the Sun are 62 AU, 430 AU, 886 AU and 8995 AU respectively. To put this into perspective, Pluto orbits the Sun at an average distance of 39 AU.

So if we used our imaginations a bit, we could say that a sufficiently sized Planet X could be patrolling a snail-paced orbit somewhere beyond Pluto. But there’s an additional problem for Planet X conspiracy theorists. If there was any object of sufficient size (and by “sufficient” I mean Pluto-mass, I’m being generous), according to a 2004 publication by David Jewitt, from the Institute for Astronomy, University of Hawaii, we would have observed such an object by now if it orbited within 320 AU from the Sun.

Suddenly, the suggestion that Planet X will be making an appearance in 2012 and the crazy idea that anything larger than a Pluto-sized object is currently 75 AU away seems silly. Sorry, between here and a few hundred AU away, it’s just us, the known planets and a load of asteroids (and perhaps the odd plutino) for company.

Source: arXiv, Astroengine.com

Volcanic Ash

Ash plume from Mount Cleveland. Image credit: NASA

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When volcanoes erupt, they can release large quantities of lava, rocks, hot gasses and volcanic ash. This volcanic ash is made up of pulverized rock and glass particles smaller than 2 millimeters in diameter. Once ejected into the air, it can travel for hundreds of kilometers before coming back to Earth.

There are two kinds of volcanic ash: fine ash, with particles smaller than 0.063 mm, and course ash, with particles smaller than 2 mm. Larger rocks aren’t kept aloft and rain down around the volcano’s cone during an eruption. The largest rocks are called volcanic bombs, and they can be as large as 6 meters across.

Ash is created when solid rock shatters and magma separates into tiny particles during an explosive eruption. The violent eruption together with steam tears apart the rock surrounding the volcano’s vent, and fires it up into the air – sometimes many kilometers into the air.

Once the volcanic ash is in the air, obscures light from the Sun, turning the sky hazy and yellow. It can even make spectacular sunsets. A large enough eruption can spread volcanic ash around the world, cooling the Earth for several years. The smallest particles can be held aloft in the Earth’s atmosphere for years, and spread around the planet on high-altitude winds.

Volcanic ash is part of one of the biggest dangers with volcanoes: pyroclastic flows. These occur when hot gas and ash erupt from a volcano and flow down its flanks at high speed. These flows can have temperatures higher than 1,000 degrees C, and travel at more than 700 km/hour. It’s impossible to outrun a pyroclastic flow.

When the ash finally lands around a volcano, it can cause further problems. Just a few centimeters of ash is heavy enough to collapse roofs, and kill animals and crops. If there’s rain, the ash turns into a sticky, muddy mess that will take months to clean up.

We have written many articles about volcanoes for Universe Today. Here’s an article about different types of volcanoes, and here’s one about different types of lava.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

List of Volcanoes

Redoubt volcano crater showing rapidly melting glacier and enlarged "ice piston" feature. Picture Date: March 21, 2009 Image Creator: Cyrus Read, Image courtesy of AVO/USGS.

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There are thousands and thousands of known volcanoes around the world. Many have no names, and most are located deep underneath the ocean at the point where the Earth’s tectonic plates are spreading apart. This is just a partial list.

List of Volcanoes
Fogo Caldera, SW Cape Verde Is. Atlantic Ocean
Merapi Volcano, Java, Indonesia
Batur Voclano, Bali, Indonesia
Rabaul Caldera, Papua New Guinea
Pinatubo Volcano, Central Luzon, Philippines
Mt Canlaon, Negros Islands, Philippines
Bulusan, Luzon, Philippines
Parker, Southern Mindanao, Philippines
Gemini Seamount, New Hebrides Island Arc, Vanuatu Islands
Aoba (Ambae Island), Vanuatu Islands
Barren Island, Andaman Islands, Indian Ocean, India
Mt Unzen, Japan
Bezymianny Volcano, Kamchatka, Russia
Karymsky Volcano, Kamchatka, Russia
Klyuchevskoi Volcano, Kamchatka, Russia
Avachinsky Volcano, Kamchatka, Russia
Kilauea Volcano, Hawaii
Loihi Seamount, Hawaii
Marianis Islands
Metis Shoal, Tonga
Ruapehu, New Zealand
Taupo Volcanic Zone, New Zealand
Akutan Volcano, Aleutian Islands
Shishaldin Volcano, Aleutian Islands
Mt Spurr, Alaska
Pavlof Volcano, Alaska Peninsula
Gorda Ridge, Northeast Pacific Ocean
Mount St. Helens
Mount Lassen, California
Lake Superior Ice Volcanoes, Michigan
Popocatepetl, Mexico
Santa María Volcano, Guatemala
Pacaya Volcano, Guatemala
Fuego Volcano, Guatemala
Tacaná Volcano, Guatemala
Cerro Quemado Volcano, Guatemala
Arenal Volcano, Costa Rica
Volcano Rincon de la Vieja, Costa Rica
Coatepeque, El Salvador
Ilopango, El Salvador
Izalco, El Salvador
San Miguel, El Salvador
San Salvador, El Salvador
San Vicente, El Salvador
Santa Ana, El Salvador
Cerro Negro, Nicaragua
Soufriere Hills, Montserrat, West Indies
Galeras, Nevado Cumbal, Dona Juana, Cerro Negro de Mayasquer, Azufral
Galapagos, Fernandina
Stromboli Volcano, Italy
Etna Volcano, Italy
Bardarbunga/Grimsvotn Volcanoes, Iceland
Askja Volcano, Iceland
Krafla Volcano, Iceland
Hekla Volcano, Iceland
Katla Volcano, Iceland
Vestmannaeyjar Volcano, Iceland
Mount Erebus, Antarctica

Thanks to the list at the MTU Volcanoes Page. The best list of volcanoes is located at the Oregon State University website. And another great list from NASA.

We have written many articles about volcanoes for Universe Today. Here’s an article about dormant volcanoes, and here’s an article about extinct volcanoes.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

What are Extinct Volcanoes?

Extinct Volcano

There are three ways to describe a volcano’s activity; there can be active, dormant, or extinct volcanoes. Active volcanoes have erupted recently. A dormant volcano isn’t erupting right now, but vulcanologists expect it could erupt at any time. Extinct volcanoes haven’t erupted for tens of thousands of years, and aren’t expected to erupt again.

What causes volcanoes to go extinct? Simply put, they’re cut off from their supply of lava. This is where a chamber of magma underneath the surface of the Earth finds its way to the surface through weaknesses in the crust. A good example of this is the hotspot that created the chain of Hawaiian Islands. The tectonic plate carrying the islands is slowly moving, so that volcanoes are cut off from the hotspot underneath. Eventually they go extinct, while the hotspot creates a new volcano further to the East.

Some volcanoes look extinct, but it might just be a long time since they’ve erupted. For example, the Yellowstone Caldera in Yellowstone National Park hasn’t had a violent eruption in about 640,000 years, but scientists think it’s still active. There has been minor activity and lava flows as recently as 10,000 years ago. The region also has regular minor earthquakes and ground is lifting up in some areas, so scientists think that’s it’s still an active volcano.

Volcanoes thought to be extinct have erupted again. For example, Mount Vesuvius erupted famously in AD 79, destroying the towns of Herculaneum and Pompeii. And the Soufriere Hills volcano on the island of Montserrat resumed activity in 1995.

Other volcanoes are clearly extinct, with only the heavily eroded lava plug remaining.

We have written many articles about volcanoes for Universe Today. Here’s an article about shield volcanoes, which can sometimes be extinct. And here’s another about dormant volcanoes.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

New Documentary “400 Years of the Telescope” Now Airing


A new 60-minute documentary created especially for the International Year of Astronomy is now airing on PBS stations in the US. “400 Years of the Telescope: a journey of science, technology and thought” is a remarkable voyage through space and time, filled with stunning, high-definition footage showing not only images from space taken by observatories around the world, but also the remote and beautiful locations where our eyes on the Universe – our magnificent telescopes – sit. It also provides a tour through the evolution of telescopes since Galileo’s first astronomical observations, and how the telescope has changed our perceptions of the cosmos and ourselves. The documentary also includes interviews with scientists who helped develop the observatories, and those who have made incredible discoveries with them. Narration by astrophysicist Neil de Grasse Tyson and a beautiful original score of music complete this wonderful documentary that you won’t want to miss. Check here for airing times on your local station. This video is also available for purchase.

But the documentary doesn’t end with airing on television. This is a multi-faceted production including extensive web content and planetarium shows. Universe Today had the chance to talk with the writer/director/producer of the project, Kris Koenig of Interstellar Studios. To find out more about this entire project, enjoy our interview, below, and make sure you watch the trailer for the show, above.

Universe Today: This sounds like a wonderful project. Can you tell us more about everything that is involved with “400 Years of the Telescope?”

Kris Koenig: This is a multi-faceted production, beginning with a high-definition documentary for PBS. We’re also creating a full dome planetarium show (Two Small Pieces of Glass) that will also be stepped down to all the different formats for different planetarium domes. We’ve been filming with a 4K camera, which means the production will be able to transition to an IMAX. So there’s an IMAX program, a public television documentary, and a planetarium program. In addition to that, we are partnering with PBS affiliates around the country through a grant through the National Science Foundation that will allow us to coordinate with the Astronomical Society of the Pacific to do events throughout the year based on the initial and subsequent broadcasts of the show. We’ll be encouraging people to go to the science centers and planetariums to watch the planetarium show, and then when they step outside, there to meet them will be local astronomers with telescopes.

What we’re doing is exactly the goals of IYA, which is to educate, and encourage people to go out and have a telescopic experience. That’s what we hope to achieve with that production.

Also, we knew from the beginning that we wanted a lot of web content. We conducted over 70 hours of interviews, which of course, we couldn’t include them all in the documentary. So of those 70 hours of interviews will be available on the internet, and totally downloadable and searchable by key terms. The transcript can be downloaded; there will be footage people can watch. The footage can also be downloaded and students can create their own documentaries. So this whole project can spawn a bunch of documentaries that can be used for school projects or shown locally. So we’re trying to outreach to the arts as well as into science.

(Teachers and students –Check out this link for additional educational activities.)

UT: How long have you been working on this project?

Kris Koenig.  Credit:  400 Years of the Telescope
Kris Koenig. Credit: 400 Years of the Telescope

Koenig: In 2005, we had just finished production of a ten-hour telecourse for PBS, for which we received two Emmy’s (Astronomy Observations and Theories, distributed by Coast Learning). I was visiting with Debbie Goodwin from Keck Observatory and she asked me, “What are you doing for IYA?” I said, “IY what?” We had actually started work on another production, which we hope we can get back to. But by the end of that week we had formed our advisory board, and initially coordinated things with a PBS station. By March we had our first launch meeting where all the advisers came together and discussed what the program should be like, what should we focus on and what should we avoid. We drafted a treatment to PBS and got a letter of encouragement back and we started the production. We brought together our planetarium partners because Peter Michaud at the Gemini telescope called me after he heard about the project and proposed joining forces to develop the content for a planetarium show. We started shooting in August of 2007.

UT: Traveling around the world to capture this must have been incredible! What stands out in your mind in creating this documentary?

Koenig: I think the thing that capped the whole project happened very early on. We were in the Institute and Museum of the History of Science in Florence, and had just finished taping Galileo’s telescope. The people there, Georgio Strano and Paolo Galluzzi who came in as partners in the project agreed to pull out the telescope — which never happens; this telescope always stays in the case. They dusted it off and we shot it with every angle we could. As Georgio was going to put it back in the case, he turned to me and asked, “Would you like to look through it?” So we all got to look through it. That was a very emotional moment. I still tear up, just talking about it.
400 Years_banner. Credit: 400 Years of the Telescope
Then we shot our reenactments of Galileo in his home, and one of scenes you see is in his cellar where he recanted. Stefano Lecci, who is our actor, is the staff actor for the museum. Even though we held a city wide Galileo search, he walked in early in the morning and said, “Why are you doing a contest? I’m the guy.” And I thought, well, we’ll see. At the end of the day, I said, “You’re right. Why did we hold a contest?” He’s a great guy, and he knows the recantation by heart, and he did it in Italian. That was another very moving moment. He’s both the old and young Galileo. We had a great makeup artist. We shot old Galileo first, then middle aged Galileo, then the younger. Each time, the transition was remarkable.

We did a reenactment at Middleburg, with Copernicus, reenactments with Hans Lipperhey in Holland, and Christina Huygens. Old castles that date back the 1300’s are a very cool environment to shoot in! We had a lot of fun in Cambridge, shooting reenactments of Isaac Newton on campus, and we have him in the river, too. We have expert on Newton speaking and we pan the camera and there’s Newton rowing a punt.

Another memorable moment was being up at Mauna Kea shooting time lapse video. The laser at the Keck Telescope came on and we captured that, and we now have in our footage for our production. It was totally unplanned. It must have been 15 degrees below zero, but I just stood there. Normally I start the camera and leave, but I just stood there and watched it because it was just an amazing sight. There are always great things like that. You go out and you plan, and you know the shots you want of dome openings and telescopes turning and you want to shoot every telescope you can, but sometimes the unplanned things end up the best.

The WM Keck Telescope. Credit: APOD
The WM Keck Telescope. Credit: APOD

We ran 6 hours of tape through a camera a day. Just as astronomy is weather dependent, so too is shooting, and the light has to be there. We had some exceptional days for lighting, which created some very pretty shots.

Once, we were in a meeting with our senior reviewer at PBS, we were talking about timetables and technical issues, but they said, “We have to stop and tell you that the footage is exceptionally pretty.” I think that’s only because of the crew. Our Associate Producer Anita Ingrao and the Director of Photographer Scott Stender were phenomenal. I’ve been around observatories my whole life; I love them, and I can look at something and say, ‘that’s the shot,’ but putting someone else in there and having them see what I was seeing isn’t always the easiest thing to do. But they put faith in what I was seeing.

UT: How many people worked on the project?

Koenig: It depends on what day it is! We had a phenomenal crew. We have animators at the University of California at Chico, animators at Mirage 3 D, New Edge Studios in Atlanta, and more animators to create the planetarium shows. Anita and Scott and I mentioned did the production team in the field, Krista Shelby is an intern, and excellent audio operator. We have an excellent board of advisers that are all leaders and experts in their fields, as well as great individuals and supporters. Neil de Grasse Tyson is the narrator and we were very happy when joined the team. I think we’ve got everyone we could possibly have on the team. It’s a great project.

Everyone in the company is an astronomer or have a passion for astronomy. That’s one thing that makes us unique in this production. Everybody is into it, they understand the importance of it and have the spirit to go behind that. I think that’s what’s going to make our production stand out. We know that there are other folks doing productions for the International Year of Astronomy, but I think what will be the point of difference is that we look at the subject as astronomers and want to communicate it properly.

Click here for a list of credits for 400 Years of the Telescope.

Official website: 400 Years of the Telescope

What are Dormant Volcanoes?

Mount St. Helens erupting.

Vulcanologists classify volcanoes into three groups: active, dormant and extinct. A dormant volcano is one that isn’t currently active or erupting, but geologists think that it’s still capable of erupting.

One of the best examples of a dormant volcano is Mauna Kea, one of the five volcanoes that make up the Big Island of Hawaii. The peak of Mauna Kea is 4,207 meters above sea level, but 10,203 meters above the base of the floor of the Pacific Ocean. Geologists classify Mauna Kea in the post-shield stage of volcanic evolution. It stopped being a shield volcano about 200,000 years ago. Mauna Kea’s last eruption is thought to be 2460 BC.

Volcanoes become dormant because the Earth’s plates are constantly shifting above volcanic hotspots. Each time the hotspot reaches the surface, it creates a new volcano. The tectonic plate continues to shift above the hotspot, and eventually the volcano is shut off from the magma chamber beneath. And so the magma finds a new source to the surface, creating a new active volcano. The older volcano stops erupting and becomes dormant. Here’s more information on the active volcanoes in the world.

Dormant volcanoes do still erupt from time to time, however, sometimes with devastating results for people who thought the volcano was completely extinct.

We have written many articles about the Earth for Universe Today. Here’s an article about different types of volcanoes, and here’s an article about the most active volcanoes in the world.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

Underwater Volcanoes

3D map of underwater volcano. Image credit: NSF

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Many volcanoes start out on land, rising above the surrounding landscape. But many more volcanoes get their start at the bottom of the ocean. These underwater volcanoes, or submarine volcanoes, can eventually grow into islands that rise above the surface of the ocean.

Geologists have identified more than 5,000 active underwater volcanoes, which account for more than 75% of the total lava that erupts every year. Most of these are located along the mid-ocean ridges, where the Earth’s tectonic plates are spreading apart. Most of these are very deep underwater, and difficult to study, but some are located in more shallow water.

An underwater volcano erupts differently than a surface volcano. This is because there is an unlimited amount of water to cool down the lava. A shell of rock hardens around the lava almost immediately, creating a type of formation called pillow lava. Deeper than about 2,000 meters, the pressure of the water is so high that it can’t boil, and so underwater volcanoes are difficult to find using hydrophones.

Underwater volcanoes build up over time, and can eventually reach the surface of the ocean. This is what happened to form the Hawaiian islands. The Earth’s crust has drifted above an active vent, creating each of the islands in turn. A new Hawaiian island, Lo’ihi, is forming under the ocean about 48 km off the southeast coast of Hawaii. It’s already taller than Mount St. Helens and will breech the surface in a few hundred thousand years.

We have written many articles about the Earth for Universe Today. Here’s an article about different types of volcanoes, and here’s an article about how volcanoes form.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

Lava Flow

Lava flow on Mount Etna. Image credit: NASA

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When you think of volcanoes, you immediately think of lava flows. These are the familiar rivers of lava pouring down the sides of the volcano, burning everything in their path, covering up building and generally ruining things. Well, you might be surprised to know that lava flows are the least hazardous way a volcano can kill you.

Molten rock is much thicker than a liquid like water. Even lava flows with the least viscosity (the least thick), will only flow at a maximum speed of a few kilometers per hour. You can easily out run a lava flow, and that’s why people are rarely killed by them. Building and trees, which are stuck to the ground, aren’t so lucky.

How far the lava flow goes depends on its viscosity. Lava flows made of basalt, like you might find in Hawaii, have very low viscosity, and so they can flow as much as 4 km away from the source and have a thickness of 10 meters. Thicker lava flows only get about 1 kilometer away from the source, but can be as thick as 100 meters.

People aren’t really at risk from lava flows, but they can do a tremendous amount of property damage. If the intense heat doesn’t set your house on fire, the slow moving wall of liquid rock will certainly knock it over and crush it to pieces. Entire towns built close to volcanoes have been overrun by lava flows, destroying houses and cars, encasing everything in meters of rock. Once an eruption is over, the lava flow can take days or even years to cool down.

Engineers have tried to battle nature, coming up with all kinds of ways to stop lava flows – few successful. In Italy, engineers have installed retaining walls to try and slow down lava flows coming down the side of Mount Etna, on the island of Sicily. These walls did slow down the lava flows enough that they didn’t reach inhabited land. In Hawaii, engineers bombed narrow lava tubes, forcing the lava to lose energy. And in Iceland, firefighters sprayed water on lava flows for nearly 5 months, cooling it so that it solidified early and didn’t block an important port.

We have written many articles about volcanoes for Universe Today. Here’s an article about the tallest volcano on Earth, and here’s an article about types of lava.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

Reference:
USGS Volcanoes: Lava Flows and Their Effects

Researchers Propose New Model for the Most Eager Supernova Explosions

2005ke, a Type 1a supernova. Credit: NASA/Swift/S. Immler

Type 1a supernovae like 2005ke, above, are known to go off when one member of a star pair exceeds critical mass and kickstarts a runaway fusion reaction.

Researchers have long puzzled over why some of the explosions happen so fast. Now, a team of Chinese astronomers believes they’ve arrived at a probable cause for the earliest of the blasts.

A team of astronomers, led by Bo Wang from the Yunnan Observatory of the Chinese Academy of Sciences, have shown how the transfer of material from a ‘helium star’ to a compact white dwarf companion causes these cataclysmic events to take place. The new results appear in Monthly Notices of the Royal Astronomical Society.
Most type Ia supernovae are believed to occur when a white dwarf  (the superdense remnant that is the end state of stars like the Sun) draws matter from a companion star orbiting close by. Previous theories for the origins of a Type Ia include an explosion of a white dwarf in orbit around another white dwarf, or an explosion of a white dwarf in orbit around a red giant star. 
When the white dwarf mass exceeds the so-called Chandrasekhar limit of 1.4 times the mass of the Sun, it eventually collapses and within a few seconds undergoes a runaway nuclear fusion reaction, exploding and releasing a vast amount of energy as a type Ia supernova. Due to their high and remarkably consistent luminosities, astronomers use these events as ‘distance indicators’ to measure the distances to other galaxies and constrain our ideas about the Universe.

Scientists have confirmed more and more type Ia supernovae, and found that about half of them explode less than 100 million years after their host galaxy’s main star formation period. But previous models for these systems did not predict that they could be this young — so Wang and his team set out to solve the mystery.

Employing a stellar evolution computer code, they performed calculations for about 2600 binary systems consisting of a white dwarf and a helium star, a hot blue star which has a spectrum dominated by emission from helium. They found that if the gravitational field of the white dwarf pulls material from a helium star and increases its mass beyond the Chandrasekhar limit, it will explode as a type Ia supernova within 100 million years of its formation. 

 “Type Ia supernovae are a key tool to determine the scale of the Universe so we need to be sure of their properties,” said research team member Zhanwen Han, also from the Yunnan Observatory. “Our work shows that they can take place early on in the life of the galaxy they reside in.”

The team now plans to model the properties of the companion helium stars at the moment of the supernova explosions, which could be verified by future observations from the Large sky Area Multi-Object fiber Spectral Telescope (LAMOST).

LEAD IMAGE CAPTION: Supernova 2005ke shown in optical, ultraviolet and X-ray wavelengths. When it was captured, this was the first X-ray image of a Type 1a, and it provided observational evidence that Type Ia come from the explosion of a white dwarf orbiting a red giant star. Credit: NASA/Swift/S. Immler

Source: Royal Astronomical Society. The paper is available here.