IYA Live Telescope Today: M104, NGC 6231, NGC 55 and Comet C/2009 G1 (STEREO)

Were you tuned in to Galactic TV today? If not, you missed a real treat. The southern skies were exceptionally clear and dark. And you know what happens when you’re photon-deprived, don’t you? Darn right… We played all night. If you didn’t get a chance to see the action, don’t despair. Believe it or not, we really and truly care about giving you an opportunity to see through the eyepiece, too… That’s why we took videos of all of tonight’s objects to share. Why not step inside and have a look at the mysterious Sombrero Galaxy, beautiful open cluster NGC 6231, huge barred irregular galaxy NGC 55 and a surprise treat… Comet C/2009 G1 (STEREO)!

I couldn’t wait to get upstairs to my office today and for the skies to get dark in Central Victoria. I had a feeling that the IYA Live Telescope was going to be doing some great things and I wasn’t disappointed. First object up? M104… the Sombrero Galaxy…

The Sombrero Galaxy (also known as M104 or NGC 4594) is an unbarred spiral galaxy in the constellation Virgo. It has a bright nucleus, an unusually large central bulge, and a prominent dust lane in its inclined disk. The dark dust lane and the bulge give this galaxy the appearance of a sombrero. The galaxy has an apparent magnitude of +9.0, making it easily visible with amateur telescopes. The large bulge, the central supermassive black hole, and the dust lane all attract the attention of professional astronomers.

Sure, the Sombrero is cool and I loved every second of it. But… About the time I had my coffee finished, I had Uranometria open and digging for some southern studies. Chances are I’ll never be well enough, nor rich enough, to visit ‘down under’ so I really want to see some of these clusters with my own eyes. I want to sketch them… Log them… Look up their RA and Dec. I want to call them my own… I want to beg Bert (our intrepid volunteer at Southern Galactic Telescope Hosting who stays up all night just to aim this scope for us for free cuz’ he’s cool… ) to move that scope!

Next up? NGC 6231….

NGC 6231 is an open cluster located near Zeta Scorpii. Zeta1 and Zeta2 Scorpii are members of this star cluster. This cluster is estimated about 3.2 million years old, and is approaching the Solar System at 22 km/s. Very young stars including it, belong to the Scorpius OB association. Zeta1 Scorpii (spectral type O8 and magnitude 4.71.[1]) is hottest star in it. It was discovered by Giovanni Batista Hodierna before 1654. Hodierna listed it as Luminosae[2] in his catalogue of deep sky observations. This catalogue was included in his book De Admirandis Coeli Characteribuse published in 1654 at Palermo. It was independently observed by other astronomers after Hodierna.

Aaaaaaah…. What a beauty! Totally satisfied, I put my sketches away in my desk, logged my information and settled into work. Why be a scope hog? I logged off to give others some free air space and next thing you know? Well, Bert is tugging on my virtual sleeve and telling me to look again. Holy cow… Check this out! He’s got NGC 55 in!!

NGC 55 is a barred irregular galaxy located about 7 million light-years away in the constellation Sculptor. NGC 55 and the spiral galaxy NGC 300 have traditionally been identified as members of the Sculptor Group, a nearby group of galaxies in the constellation of the same name. However, recent distance measurements indicate that the two galaxies actually lie in the foreground. It is likely that NGC 55 and NGC 300 form a gravitationally bound pair.

Well, I didn’t think anything could top that. I watched fascinated as the pencil slim galaxy filled the whole screen and the nucleus would scream in and out. I couldn’t believe how huge it was! Structure… my word… We’ve got structure coming out of an edge-on galaxy in a little bitty scope set on the edge of the world. So, I start digging around for my pencils and paper again. More sketches? Yeah. More sketches.

Then Bert really lays one on me. He’s going to try for something even I wouldn’t dream our little IYA scope could pick up. He asks me for some information and brother? I’m on it. I guarantee you within 180 seconds we both had the epoch and charts ready and I even had the coordinates. The instant message said he had to stop for a few minutes to dark adapt and we were going for it… Could it be? Could it happen? Yeah. It did.

Our final target for the day was Comet C/2009 G1 (STEREO). At magnitude 10.2 (RA 0h 37m 26s Dec 37°36’6″) we weren’t going to set any records for showing it bright and beautiful – but considering we’re running with an 80mm scope, we aren’t doing too bad! It’s faint, but it’s darn near center and if you’re good at the eyepiece? You can’t miss it.

Have a look…

Comet C/2009 G1 was discovered by Jiangao Ruan of China who found the 10th magnitude fuzz ball on images taken by the SECCHI HI-1B instrument onboard one of the STEREO spacecraft. Since the comet was discovered in spacecraft data it was naturally named after the spacecraft – and thus the name STEREO. Pretty cool considering the data is public domain and the person who caught it out was an amateur watching what was going on! Congratulations to Jiangao on his 19th find from SOHO and STEREO data in less than a year!

So, while Bert filmed the video for you to try and capture the movement of the comet, I called every comet watcher I knew on the telephone and we were all glued to our monitor screen sketching this comet and comparing star charts and logging the stars for our records. Once crazy? Always crazy. I guess even having a Comet Hunter’s Gold Medal hasn’t stopped the fever! (Hopefully those of you who are also working on your AL comet studies will take the clues I’ve left you and do the same!)

Well, I hope you had as much fun viewing the videos as we did taking them for you! As always, check the IYA Live Telescope for broadcasts whenever you get a chance. We’re working on picking up other observatories around the world and maybe before the end of the year we’ll even be running something 24/7! (yeah, rite… like there’s somewhere in the world that’s not cloudy all the time?)

Italicized information is a direct quotation from Wikipedia and we appreciate it!

Disappearing Accretion Disk Is Missing Link in Pulsar Birth

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A now-you-see-it, now-you don’t accretion disk (white and blue in the artist’s rendering at left) has tipped astronomers to the birth of a superfast, “millisecond” pulsar that was happening right before their eyes — er, their radio telescopes.

The new finding confirms the long-suspected evolutionary connection between a neutron star and a millisecond pulsar: they are two life stages of the same object.

Anne Archibald, of McGill University in Montreal, Canada and her colleagues announced their discovery in the May 21 online issue of the journal Science.

Pulsars are superdense neutron stars, the remnants left after massive stars have exploded as supernovae. Their powerful magnetic fields generate lighthouse-like beams of light and radio waves that sweep around as the star rotates, and are detectable as pulses on Earth.

Some, dubbed millisecond pulsars, rotate hundreds of times a second. Astronomers believe the fast rotation is caused by a companion star dumping material onto the neutron star and spinning it up.

The material from the companion would form a flat, spinning disk around the neutron star, and during this period, the radio waves characteristic of a pulsar would not be seen coming from the system. As the amount of matter falling onto the neutron star decreased and stopped, the radio waves could emerge, and the object would be recognized as a pulsar.

This sequence of events is apparently what happened with a binary-star system some 4000 light-years from Earth, in the constellation of Sextans just south of Leo. The millisecond pulsar in this system, called J1023, was discovered by the National Science Foundation’s Robert C. Byrd Green Bank Telescope (GBT) in West Virginia in 2007 in a survey led by astronomers at West Virginia University and the National Radio Astronomy Observatory.

The astronomers then found that the object had been detected by National Science Foundation’s Very Large Array radio telescope in New Mexico, during a large sky survey in 1998, and had been observed in visible light by the Sloan Digital Sky Survey in 1999, revealing a Sun-like star.

When observed again in 2000, the object had changed dramatically, showing evidence for a rotating disk of material, called an accretion disk, surrounding the neutron star. By May of 2002, the evidence for this disk had disappeared.

“This strange behavior puzzled astronomers, and there were several different theories for what the object could be,” said Ingrid Stairs of the University of British Columbia.

The 2007 GBT observations showed that the object is a millisecond pulsar, spinning 592 times per second.

“No other millisecond pulsar has ever shown evidence for an accretion disk,” Archibald said. “We know that another type of binary-star system, called a low-mass X-ray binary (LMXB), also contains a fast-spinning neutron star and an accretion disk, but these don’t emit radio waves. We’ve thought that LMXBs probably are in the process of getting spun up, and will later emit radio waves as a pulsar. This object appears to be the ‘missing link’ connecting the two types of
systems.”

The scientists have studied J1023 in detail with the GBT, with the Westerbork radio telescope in the Netherlands, with the Arecibo radio telescope in Puerto Rico, and with the Parkes radio telescope in Australia. Their results indicate that the neutron star’s companion has less than half the Sun’s mass, and orbits the neutron star once every four hours and 45 minutes.

Image caption: Material from distended “normal” star. right, streams onto accretion disk (white and blue) surrounding neutron star, left. Credit: Bill Saxton, NRAO/AUI/NSF

Source: National Radio Astronomy Observatory. Animations are here and here. Warning: that last one may cause dizziness.

With Moon Rocks in Hand, Parazynski Reaches Mt. Everest Peak

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We’ve been following former astronaut Scott Parazynski’s attempt to climb Mt. Everest, and now comes the news that he has successfully reached the summit, one year after a back injury forced him to give up his climb. “It was a wonderful experience, though and through,” Parazynski said in a Skype interview with Miles O’Brien, “and certainly the most challenging thing I’ve ever done in my life, both physically and mentally.” Parazynski brought several objects with him to the world’s highest summit, including rocks from the Moon, and remembrances of fallen astronauts. Parazynski is the first astronaut to summit Mt. Everest.

During the climb, Parazynski was doing research. “We’ll be collecting data for astrobiologists, looking for extremophile life,” Parazynski told Universe Today in an interview before he left for Mt. Everest. “If you understand how extremophiles live, you might be able to understand how life may have once evolved on Mars, or may still exist on Mars.”

Scott Parazynski on the summit of Mt. Everest.  Credit: OnOrbit.com
Scott Parazynski on the summit of Mt. Everest. Credit: OnOrbit.com

Parazynski tested NASA-derived hardware, taking along a prototype lunar geology camera and other hardware for extreme environments. “Up high on the mountain there are limestone formations, which are wonderful places to look for fossilized life,” he said,” and we’ll also look for melt water and primitive forms of life there; algae lichens, etc. If liquid water exists even for brief periods on Mars it may be in similar conditions to what we’ll find on Mt. Everest. We hope to bring samples back for scientists to look at.”

Now that he has successfully reached the summit, Parazynski said he won’t return to Everest. “Once is enough,” he said, adding that his family is glad he now has the bug to climb Everest out of his system.

Check out all the videos of Parazynski’s climb at Miles O’Brien’s blog at True/ Slant, as well as more images from Keith Cowing at On Orbit.com. Congratulations to Scott Parazynski!

And I just had to share this image of Parazynski on the summit after the sun rose. It looks just like Luke Skywalker on the planet Hoth at the beginning of “The Empire Strikes Back.”

Scott  Parazynski at the summit.  Credit:  OnOrbit.com
Scott Parazynski at the summit. Credit: OnOrbit.com

Look for an upcoming special on the Discovery channel about Parazynski’s climb.

A Brotherhood of Hubble Warriors: Jeff Hoffman Reflects on HST Repair Missions

Hoffman, on the robotic arm, works with Story Musgrave on an EVA on STS-61. Credit: NASA

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Not surprisingly, former astronaut Jeff Hoffman has been watching the current Hubble servicing mission with interest. After all, he was a member of the first repair crew that visited the telescope in December 1993, part of the team which essentially rescued the Hubble program from what could have been a disaster. But, now Hoffman is impressed with this current crew and what they’ve accomplished, saying they are part of a “brotherhood of Hubble warriors.”

And Hoffman is feeling a little nostalgic, too.

“It certainly brought me back 15 years to when I was doing that job,” he told Universe Today. “I look at them floating around Hubble, seeing images from their helmet cameras and watching them work with all those tools, and I feel a little heart tug. But also, I feel tremendous excitement because every time we go up there we just make Hubble better and better. It’s just a phenomenal story.”

Hoffman installing WFPC2 on Hubble.  Credit: NASA
Hoffman installing WFPC2 on Hubble. Credit: NASA

One of Hoffman’s tasks on the first Hubble repair mission, STS-61, was to install the Wide Field Planetary Camera 2. Later nicknamed “The Camera that Saved Hubble,” WFPC2 replaced the original optical camera on Hubble, and was constructed to work with the corrective optics instrument (COSTAR) – basically a set of eyeglasses to overcome the spherical aberration in Hubble’s primary mirror.

“I put the Wide Field Planetary Camera 2 in Hubble in 1993,” Hoffman reminisced, “and that is the camera that has taken the majority of the spectacular pictures by which the whole world has come to know Hubble. This crew has removed it now and replaced it with an even more powerful camera. So I had kind of a bittersweet moment when I saw “my camera” leaving the telescope!”

But he said he is looking forward to seeing even more spectacular images from WFPC3. Plus, Hoffman has been invited to Goddard Space Flight Center to see his old camera when it returns from space. “I’ll get to put my hands on it once again after fifteen years.”

Astronaut Jeffrey A. Hoffman, floating in the forward middeck area,   displays tools used in the five space walks on STS-61.  Credit: NASA
Astronaut Jeffrey A. Hoffman, floating in the forward middeck area, displays tools used in the five space walks on STS-61. Credit: NASA

For Hoffman, what is most remarkable about the current mission was the type of work the astronauts were able to do, and the panoply of tools they had at their disposal. “One of the fantastic developments is the ability for astronauts to do complex servicing, and the tools are really what make these tasks possible,” he said. “Wearing astronaut gloves, you are really pretty clumsy. It’s like wearing welder’s gloves or ski mittens and trying to do brain surgery. But the engineers have now developed a whole suite of tools optimized for the individual tasks, allowing what would otherwise be impossible to come within the realm of what an astronaut dressed in a spacesuit can accomplish.”

The electronics on two of Hubble’s instruments had failed, — the Space Telescope Imaging Spectrograph (STIS) and the Advanced Camera for Surveys (ACS) — and the STS-125 crew basically went into the electronic guts of both instruments, pulled out circuit boards and replaced them.

Seeing the astronauts make repairs at that level was a marvel, Hoffman said. “That is something which we never imagined doing with Hubble. But it just shows how with every mission we’ve gotten more and more willing to push the envelope.”

Dr. Jeffrey Hoffman. Credit: NASA
Dr. Jeffrey Hoffman. Credit: NASA

Hoffman retired from NASA in 1997 and is now a professor of aeronautics and astronautics at MIT. He believes Hubble’s greatest legacy is how the observatory has impacted society.

“People all over the world have developed a love for Hubble,” he said, “and from Hubble we have the knowledge that the Universe is a stranger and more beautiful place that any of us had ever imagined. That’s what Hubble has done for people, giving us breathtaking images that are in some cases more beautiful than any abstract artist could come up with.”

But it’s not just the beautiful pictures. “The power of Hubble to show us what the Universe is like just one or two billion years after the Big Bang, where we can actually see the birth of the first few galaxies that were forming in our universe — this is mind boggling stuff. Hubble has re-written astronomy textbooks over the years and with the new set of instruments having even more sensitivity, it’s going to happen all over again.”

Hubble floating away after being released by the STS-61 crew in 1993.  Credit: NASA
Hubble floating away after being released by the STS-61 crew in 1993. Credit: NASA

Now that the current crew has released Hubble, Hoffman recalled watching the telescope float away after the completion of his own mission. “They were probably looking at it with the same feeling of nostalgia as we did as we watched it slowly drift away,” he said. “It’s kind of a fraternity of Hubble, all the people in the six crews who have been involved with the Hubble Space Telescope. Every time I see someone from the crews that have worked on Hubble or the thousands of people on the ground who have been involved with it over the years, it’s like a brotherhood/sisterhood of Hubble warriors, so to speak. It’s been just an incredible adventure and it is nowhere near the end yet. I look forward to another 5, 10, maybe 15 years of incredible discoveries coming down from the Hubble Space Telescope.”

IYA Live Telescope Today: Jupiter and Neptune Conjunction – M19

Hey, hey! We’re baaaack… Due to some technical difficulties, our eye on the southern sky has been down for a short time, but I’m happy to report that we’re back up and running again. If you missed our broadcast yesterday and today, have no fear. We recorded the Jupiter and Neptune conjunction for you and captured Messier 19 today, too! Come on… You know you want to look!

Even though it only looks like two dots hanging out on a black background, it’s knowing what those two dots are that counts. In order to get them both in the same frame, we used minimal magnification. Jupiter is the brightest and will appear at the bottom of the frame, while Neptune is fainter and at the top of the frame.

Ready for the next? Then step up to the eyepiece and view Messier Object 19….

(The following is a cut and paste from Wikipedia)

Messier 19 or M19 (also designated NGC 6273) is a globular cluster in the constellation Ophiuchus.

It was discovered by Charles Messier in 1764 and added to his catalogue of comet-like objects that same year.

M19 is the most oblate of the known globular clusters. It is at a distance of about 28,000 light-years from the Solar System, and is quite near to the Galactic Center, at only about 5,200 light-years away.

As always, you can visit the remote telescope by clicking on the IYA “LIVE Remote Cam” Logo to your right. Just remember if you get an error message, that means it is either daylight or cloudy… Or the scope or broadcasting system is dead and so are the volunteers running it. We’ll be broadcasting whenever skies are clear and dark in Central Victoria! Enjoy…

Factual information is copied from Wikipedia. Thank you so much!

Where In The Universe #55

Are you ready for another Where In The Universe Challenge? Take a look and see if you can name where in the Universe this image is from. Give yourself extra points if you can name the spacecraft responsible for the image. As usual, we’ll provide the image today, but won’t reveal the answer until tomorrow. This gives you a chance to mull over the image and provide your answer/guess in the comment section. Please, no links or extensive explanations of what you think this is — give everyone the chance to guess.

UPDATE: The answer has now been posted below. Don’t peek before you make your guess.

What you are seeing here is the dark side of Saturn’s moon Titan, with sunlight filtering through the moon’s hazy atmosphere. And obviously, the Cassini spacecraft is responsible for this image.

An airless satellite would appear in this viewing geometry only as a lit crescent. But Titan’s thick atmosphere scatters light around all edges of the planet to create a ring of light.

This view looks toward the Saturn-facing side of Titan. North on Titan is up and rotated 45 degrees to the left. The images were acquired at a distance of approximately 1.8 million kilometers (1.1 million miles) from Titan and at a Sun-Titan-spacecraft, or phase, angle of 157 degrees. Image scale is 11 kilometers (7 miles) per pixel.

Nice job, everyone! Check back next week for another WITU challenge!

SRB Videos, A Toast to Recycled Urine and Other Misc. Spaceflight Notes

ISS crew drinks recycled water. Credit: NASA TV


It has been a busy day in space and here are a few jottings about what all has been going on. Above, you can watch the spectacular videos taken by cameras mounted on the shuttle’s solid rocket boosters, taken during the launch of Atlantis on the current Hubble Servicing Mission. It’s a crazy ride, tagging along on the outside of the shuttle going up, and spinning dizzily on the way down until splashing in the ocean. Not for the faint of heart! But seeing the SRB videos means only one thing: Atlantis and the STS-125 crew have been cleared to land. NASA has carefully reviewed the videos and the data from the crew’s scan of the shuttle’s thermal protection system, saying there are absolutely no issues that would preclude the shuttle from landing. Weather, however could be another matter, which is why NASA ordered the shuttle to power down for awhile today to save on consumables. Predicted weather does not look good for landing on Friday, so the crew will make sure they have enough power to stay in orbit for a few more days.

Now about that toast…

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A huge crowd gathered in the space station mission control room at Johnson Space Center today as the ISS crew was given a “go” to drink water that the new recycling system has purified. Everyone joined in at mission control with a toast to the success of the recycling system, giving a nod to everyone who helped create the system, install it on the ISS and work on getting the fussy system to run. This is big news, as it means the station is ready to handle the increased crew size of 6 astronauts.

Also:

The STS-125 crew held a press conference from the shuttle today. The highlight was Mike Massimino talking about how he ripped a handrail off of Hubble in order to proceed with the scheduled repair of the STIS instrument.

“Ripping that thing out of there was quite an experience, and I’m glad it led to a successful repair,” said Massimino, who added that he drew inspiration from his uncle Frank, who once ripped an oil filter out a car. “That was pretty close to what was going on with Hubble.”

Later, during a ship-to-ship call between Atlantis and the ISS, space station crew member Michael Barrett revisited Massimino’s special touch.

“The magic Massimino touch is now legendary, and we’re looking forward to seeing you guys back on the ground,” he said.

If you missed the crew news conference, its available here. Additionally, the discussion between the two crews, can be seen here.

Update: One other piece of news from the shuttle is that President Obama called the STS-125 crew to congratulate them on a job well done. “I wanted to personally tell you how proud I am of all of you and everything that you’ve accomplished,” he said.

“Like a lot of Americans, I’ve been watching with amazement the gorgeous images you’ve been sending back and the incredible repair mission you’ve been making in space,” he said. “I think you’re providing a wonderful example of the kind of dedication and commitment to exploration that represents America and the space program generally. These are traits that have always made this country strong and all of you personify them.”

Obama also said he would be naming a new NASA administrator very soon, but wouldn’t say who it is.

“Just so we’re sure, the new administrator is not any of us on the flight deck right now, is it?” asked Commander Scott Altman (Altman had suggested Hubble fix-it man John Grunsfeld for administrator earlier this week.)

“I’m not going to give you any hints,” Obama said with a laugh.

“Thank you very much, fair enough, sir,” Altman replied.

Listen to the audio and/or read the transcript of Obama’s call here.

One other spaceflight news tidbit, Orbital Sciences Corp. finally launched a Minotaur 1 rocket from the Wallops Island Flight Facility with the Tactical Satellite-3 (TacSat-3) satellite. The launch was heavily postponed, with several scrubs relating from the weather to the launch vehicle and facility. Find out more about the launch and the satellite here.

Volcano Caldera

Crater Lake in Oregon. Image credit: Zainubrazvi

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A volcano caldera is a depression in the ground created by the collapse of land after a volcanic eruption. In some cases, the caldera is created slowly, when the ground sinks down after a magma chamber is emptied. In other situations, the magma explodes violently, and the caldera is the deep pit in the ground that remains after the volcano blows its top off.

A caldera forms when the magma chamber beneath a volcano is emptied in a large eruption. If the eruption happens quickly enough, the empty chamber beneath isn’t strong enough to support the weight of the volcano and it collapses down. This can happen in a single cataclysmic event, or over the course of several eruptions. Volcano calderas can be hundreds and even thousands of square kilometers in area.

There are many famous examples of volcano calderas. Crater Lake in Oregon was created when a volcano detonated around 10,000 years ago. Over time water filled up the nearly 597 meter deep caldera, making it the deepest lake in the United States, and the second deepest lake in North America (Great Slave Lake is the deepest). Another example of a volcanic caldera is the Yellowstone Caldera, which last erupted 640,000 years ago. It released 1,000 cubic kilometers of rock, covering much of North America in two meters of debris.

There are other examples of non-explosive volcano calderas. For example, the volcano Kilauea on the Big Island of Hawaii has a magma chamber that’s emptied by large lava flows, and not explosive eruptions. This causes the ground to collapse down after the lava eruptions, sinking many meters into the ground.

Volcano calderas have been seen on many other places in the Solar System. Although there aren’t active volcanoes on Mars today, regions of Mars were active billions of years ago, and there are many regions with large calderas. Jupiter’s moon Io is an example of a place with active calderas being created right now.

We have written many articles about volcanoes for Universe Today. Here’s an article about types of eruptions, and here’s an article about volcanic craters (not to be confused with calderas).

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.

References:
http://vulcan.wr.usgs.gov/Volcanoes/CraterLake/Locale/framework.html
http://volcanoes.usgs.gov/yvo/about/faq/faqhistory.php
http://hvo.wr.usgs.gov/gallery/kilauea/caldera/main.html

Volcano Crater

Volcano Crater. Image credit: Dirk van der Made

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Some craters are formed by a meteor impact, when a space rock strikes the Earth. And other craters are volcanic in origin. A volcano crater is a circular depression around a volcanic vent. This is where the lava, ash and rock erupt out of a volcano. In most situations, the volcano crater is located at the top of the volcano.

Think of a classic cone-shaped volcano, with steep sides and a slightly flattened top. If you could climb up to the top of the volcano and peer over the edge, you would look down into the volcano crater. And when the volcano does erupt, the material comes out of this volcano crater.

But not all volcano craters are found at the top of the volcano. They can also appear on the flanks of large volcanoes, when side vents reach the surface and erupt. These are known as flank craters, while the crater on top is called a summit crater. The volcano crater will often fill up with water and create a crater lake.

One kind of eruption creates a crater without a volcanic cinder cone at all: a phreatic eruption. This is a situation where magma rises through water-saturated rocks and causes steam to build up under the surface. The pressure from all the steam causes the rock to explode outward and create a volcanic crater. These can be strange to discover as they often appear in plains, far away from any other obvious volcanoes.

When the ground depresses down because a volcano’s magma chamber has been emptied, this is actually known as a caldera, and not a volcano crater.

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

Ring of Fire Volcanoes

Ring of Fire Volcanoes

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The Pacific Ring of Fire is a region that surrounds the Earth’s Pacific Ocean, and is known for its volcanoes and earthquake activity. The Ring of Fire has a total of 452 volcanoes, and has 75% of the Earth’s active and dormant volcanoes. The whole Ring of Fire stretches for 40,000 km in length.

The Ring of Fire is created by the Earth’s plate tectonics. The Earth’s crust is broken up into plates which float on top of the mantle. When these plates come together, you can get volcanoes and earthquakes. The eastern side of the Ring of Fire has the Nazca Plate and the Cocos Plate being subducted (going underneath) the South American Plate. And in the North, the Pacific Plate and the Juan de Fuca Plate are being subducted underneath the North American Plate. The Pacific plate is also subducting underneath the Kamchatka Peninsula and Japan.

Because of all this subduction, there are many cracks in the Earth’s crust where magma can reach the surface and erupt as volcanoes. There are volcanoes in Chile, Mexico, the United States, Canada, Russia, Japan, the Philippines, Indonesia, New Zealand and Antarctica.

Some of the most famous volcanoes on Earth are in the Ring of Fire. A famous volcano, Mount St. Helens, which erupted in 1980 is a good example, or Mount Rainier in Washington State, or Mount Shasta in California. The recent eruption of Mount Redoubt in Alaska is part of the Ring of Fire. And so are Mount Pinatubo in the Philippines and Mount Fuji in Japan.

The Ring of Fire has produced more than just volcanoes. It has also created islands and mountain chains around the Pacific Ocean. The Aleutian Islands in Alaska are all volcanic, and Japan is part of the subduction of the Pacific Plate going underneath the Eurasian Plate.

I personally live in the Ring of Fire, so I’m aware that there are dangers to living in this part of the world. There can be powerful earthquakes, huge tsunami, and new volcanic eruptions. Every year the Ring of Fire volcanoes demonstrate just how active they still are.

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

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:
http://vulcan.wr.usgs.gov/Glossary/PlateTectonics/Maps/map_plate_tectonics_world.html