Mount Pinatubo

Mount Pinatubo is an active stratovolcano on the island of Luzon in the Philippines, and the site of one of the most powerful recent eruptions. In June 1991, the volcano produced the second largest terrestrial eruption of the 20th century (after Novarupta), and the largest eruption in living memory. At least 800 people lost their lives in the eruption, but this was lower than it could have been because of an organized evacuation effort.

Pinatubo is located in the Cabusilan Mountain range, located on the west coast of the Island of Luzon. It’s a stratovolcano made up of successive layers of andesite and dacite. Its richly forested slopes were home to several thousand indigenous people. Before the eruption, it rose to an elevation of 1745 meters, but now it’s only 1485 meters tall.

Scientists had many warnings that Pinatubo was about to erupt, and this allowed such a thorough evacuation. On July 16, 1990, a magnitude 7.8 earthquake struck about 100 km north of Pinatubo. And then in March/April 1991, molten rock was detected rising to the surface from more than 32 kilometers beneath Pinatubo. This triggered more small earthquakes through April, May and early June.

On June 12, 1991, millions of cubic meters of magma reached the surface, beginning several days of eruptions. Even more magma reached the surface on June 15th, ejecting more than 5 cubic kilometers of material. An ash cloud rose 35 kilometers into the air, covering the surrounding region in meters of ash. Dangerous pyroclastic flows of hot ash, rock and water surged down the sides of the volcano, destroying everything in their path. The huge eruption gouged out a caldera 2.5 km across.

The eruption was so significant that the ash darkened the atmosphere, and caused worldwide temperatures to drop by 0.5 degrees C.

We have written many articles about volcanoes for Universe Today. Here’s an article about Mount St. Helens, and here’s an article about Krakatoa.

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.

Newsflash: Sunspot Appears!

Sunspot animation of Sunspot 1019. Credit: Spaceweather.com

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OK, I admit – the headline is a little over the top. But the sun has been so quiet of late, that even a small sunspot can be exciting. There’s been some debate whether this period of extreme solar calm is truly unusual, or just part of the natural cycle. But solar cycle models never predicted this low amount of activity. “It turns out that none of our models were totally correct,” admitted Dean Pesnell of the Goddard Space Flight Center, a member of an international panel of experts that are now trying to predict what the next solar cycle will hold. “The sun is behaving in an unexpected and very interesting way.”

The panel is predicting that the next cycle, Solar Cycle 24 will have a peak sunspot number of 90, the lowest of any cycle since 1928 when Solar Cycle 16 peaked at 78.
Sunspot cycles

Right now, the solar cycle is in a valley–the deepest of the past century. In 2008 and 2009, the sun set Space Age records for low sunspot counts, weak solar wind, and low solar irradiance. The sun has gone more than two years without a significant solar flare.

“In our professional careers, we’ve never seen anything quite like it,” says Pesnell. “Solar minimum has lasted far beyond the date we predicted in 2007.”

For 2009, the number of “spotless” days are 123, as of May 31, which is 82%.

There’s a little sign of action on the sun, though. In recent months small sunspots and “proto-sunspots” are popping up with increasing frequency. Enormous currents of plasma on the sun’s surface (“zonal flows”) are gaining strength and slowly drifting toward the sun’s equator. Radio astronomers have detected a tiny but significant uptick in solar radio emissions. All these things are precursors of an awakening Solar Cycle 24 and form the basis for the panel’s new, almost unanimous forecast.

According to the forecast, the sun should remain generally calm for at least another year. This calm has a greater affect on Earth’s atmosphere than you might imagine. With low solar activity, the Earth’s atmosphere can cool and contract. Space junk accumulates in Earth orbit because there is less aerodynamic drag; hence the increase in the number of collision event “alarms” for the ISS and shuttles. The calm solar wind whips up fewer magnetic storms around Earth’s poles. Cosmic rays that are normally pushed back by solar wind instead intrude on the near-Earth environment. There are other side-effects, too, that can be studied only so long as the sun remains quiet.

But the sun is a very chaotic place, and even a below-average cycle is capable of producing severe space weather from solar flares and coronal mass ejections (CME) said Doug Biesecker of the NOAA Space Weather Prediction Center. So we shouldn’t be lulled into a false sense of security.

Sources: Science@NASA, SpaceWeather.com

Mount St. Helens

Eruption of Mount St. Helens

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The most powerful and devastating volcanic eruption in the history of the United States was the explosion of Mount St. Helens. This active stratovolcano, located in Skamania County, Washington detonated on May 18, 1980, killing 57 people, destroying hundreds of homes, and flattening hundreds of square kilometers of forest. The eruption tore off the top of the mountain, reducing its height from 2,950 meters to 2,550 meters.

Mount St. Helens is just one volcano in the Cascade Range of mountains that stretch down the west coast of North America. There are many other famous volcanoes in this region, like Mount Ranier, Mount Hood, and Mount Shasta. Helens is a large eruptive cone made up of several layers of lava rock interlaced with ash, pumice and other deposits. There are layers of basalt and andesite, and several domes of dacite lava have broken through.

Scientists believe that Mount St. Helens started forming about 40,000 years ago, and it’s considered the most active volcano in the Cascade Range. Before its eruption, St. Helens was the 5th-highest peak in Washington state; it was nicknamed the Mount Fuji of America. It measures about 10 km across the base and rose about 1,500 meters above the surrounding landscape.

And so, on May 18, 1980, Mount St. Helens erupted catastrophically, after nearly 2 months of local earthquakes and steam eruptions – scientists measured more than 10,000 minor earthquakes leading up to the eruption. But it was a magnitude 5.1 earthquake on May 18th that caused the volcano’s bulging north flank to slide away in the largest landslide in recorded history. This released a huge blast of hot gas, steam and rock debris that swept downhill from the summit. This pyroclastic flow melted snow and ice on the mountain, which added to the torrent of material streaming down the river valleys leading from the volcano. A plume of ash rose 19 kilometers into the air, covering 57,000 square kilometers of the Western United States.

Mount St. Helens is still active, and scientists have discovered dozens of extrusions of thick, pasty lava. A new dome is taking shape. It’s now about 1,100 meters in diameter and 250 meters tall.

We have written many articles about volcanoes for Universe Today. Here’s an article about Kilauea in Hawaii, and here’s an article about Krakatoa.

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/MSH/May18/summary_may18_eruption.html
http://vulcan.wr.usgs.gov/Volcanoes/MSH/Publications/Bulletin1859/eruption_may18_1980.html

Capture the Universe with Phil Plait

So, you think you’re a great astrophotographer? Then this is for you: the Bad Astronomer announced today he is hosting an astrophotography contest, sponsored by Discover Magazine and Celestron Telescopes. Phil himself will be the judge, so all you need to do is figure out what images he really likes and then get snapping! There are some great prizes:
Grand Prize: Celestron NexStar 8SE Computerized Telescope – Retail Value $1,399
One Runner-Up Prize: Celestron Axiom LX 31mm Eyepiece – Retail Value $399
One Viewer’s Choice: Celestron FirstScope – Retail Value $49.99
Read the rules and enter here. The only stickler-type rule is that the images need to be taken with Celestron equipment, but the contest runs from today (June 1) through June 30. Good luck to everyone, and I can’t wait to see all the images!

Kilauea Volcano

Lava fountain in Hawaii.

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The Hawaiian Island chain is a long string of islands that actually stretches for thousands of km. All of these islands were formed by the movement of the Pacific plate above a volcanic hotspot. As the plate is constantly slowly moving, it allowed volcanic islands to form and then carried them away so they would become extinct. There are 5 shield volcanoes on the Big Island of Hawaii, with Kilauea being the newest and most active.

Kilauea is located on the Eastern edge of the Big Island of Hawaii. It rises only 1,247 km above sea level; a fraction of its neighbor Mauna Loa, which rises to 4,169 km. It’s classified as part of a family of low, broad volcanoes known as shield volcanoes. The basaltic lava that erupts out of shield volcanoes has a low viscosity which can flow for dozens of kilometers. While the other volcanoes on the island are extinct or dormant, Kilauea is in an almost constant state of eruption.

Scientists used to think that Kilauea was a satellite volcano of the larger Mauna Loa, but better research has shown that Kilauea has its own magma plumbing system, starting more than 60 km below the surface of the Earth. Kilauea has almost continuous activity during the 19th century, and there were 34 eruptions since 1952. In January 1983, eruptions began along the east rift zone and haven’t stopped since.

Kilauea is one of the most accessible volcanoes in the world. You can drive right up to it, park, and walk down a short trail to peer into the volcano crater. There’s even a lodge on the ridge that gives an amazing view of the volcano. One of the best ways to view Kilauea is by boat. Tours will take visitors just offshore, where hot lava is pouring out of Kilauea and into the Pacific Ocean. This creates huge plumes of steam.

The inhabitants of the Hawaiian Islands believed that the goddess of volcanoes, Pele, lived in Kilauea. They thought that eruptions happened when their goddess was angry, and they developed many tribal chants to try and calm her down. Several unique lava formations are named after her, like Pele’s tears (small drops of lava that cooled in mid air during an eruption), and Pele’s hair (strands of volcanic glass).

We have written many articles about volcanoes for Universe Today. Here’s an article about Mount Vesuvius, and here’s an article about Mount Etna.

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 Volcano Information Page: Kilauea

Krakatoa

Illustration of the Krakatoa eruption.

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Perhaps the most famous volcanic eruption in recent history is the explosion of the volcano Krakatoa in 1883. On August 27 a series of four explosions almost entirely destroyed the island. People as far away as Perth in Western Australia could hear the detonation, and it’s estimated that 120,000 people died from the eruption. In fact, the entire climate of Earth was affected for several years after the eruption, as global temperatures dipped for 5 years.

What’s left of Krakatoa is a small group of islands located in the Sunda Strait, which divides Sumatra from the Island of Java. It’s located directly above the subduction zone of the Eurasian Plate and the Indo-Australian Plate, where the plates make a change in direction. It’s believed that the volcano’s caldera collapsed in 416 AD, forming a 7-km wide caldera. The remnants of this eruption formed Verlaten and Lang Islands. Three volcanoes (Rakata, Danan and Perbuwatan) came together to form the pre-1883 Krakatau island.

Krakatau was made up of one or more stratovolcanoes that went through 5 major periods. The first was an early growth phase, followed by the formation of the caldera. Then the caldera collapsed, and was destroyed during the 1883 eruption. A new growth phase began in December 27, and even now Krakatoa is growing by more than 12 cm/year.

The destruction of Krakatoa began on May 20, 1883 when a mild ash and steam eruptions started up. There were similar eruptions for about 3 months, and at times several vents were erupting at the same time. On August 11, large ash columns rose from the main crater of Perbuwatan. These small eruptions intensified over time, leading to the August 27th explosion that caused the collapse of the caldera.

Although the eruption of Krakatau was devastating, scientists think that many people lost their lives from the giant tsunami generated by the eruption. The largest wave reached 40 meters and killed around 34,000 people. In one case, a ship was carried 2.5 kilometers inland and dumped into the forest.

Scientists measuring the strength of volcanic eruptions using a scale called the Volcanic Explosivity Index (VEI). The eruption at Krakatau measured VEI 6 on the scale, and ejected 16 cubic kilometers of material. Anything within 16 km was covered with 16 meters of ash. Even towns located more than 450 km away were coated with a few cm of ash.

We have written many articles about volcanoes for Universe Today. Here’s an article on Mount Etna, and here’s an article on Mount Vesuvius.

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/Indonesia/description_krakatau_1883_eruption.html
http://hvo.wr.usgs.gov/volcanowatch/2003/03_05_22.html

The Truth About NASA’s UFO Videos

Image from the STS-80 shuttle mission. Taken from: AboveTopSecret

Perusing You Tube, there are lots of UFO videos, which are usually grainy, shaky videos showing nothing that can be proved definitively. But there are a couple of videos that are different — and have generated a lot of interest — because they were filmed by NASA astronauts during space missions.

I’d like to recommend everyone read an article published today by Popular Mechanics where the astronauts who were behind the camera for two of these videos speak out about what is actually in the videos, and NASA’s supposed “cover-up.” The two astronauts, Tom Jones and Mario Runco “reveal” what the videos are really showing.

“There’s no way to keep people from using public domain footage for silly purposes,” former astronaut Tom Jones says in the article. “If a shuttle beams back 10 hours of Earth views each day, there are bound to be images and scenes that are misunderstood or taken out of context.”

And “out of context” is what many UFO theories and proponents rely on, says writer Erik Sofge. And NASA tends to never make official statements debunking any of the UFO claims, which helps fuel the flames. One clip, taken by Runco is of the PAM-STU satellite that Runco and his crew deployed during the STS-77 mission in 1996, outfitted with reflective materials. During the entire clip, however, Runco or mission control never says exactly what they are filming, but keep referring to it as “the target,” typical for pilots and NASA astronauts. There are other oddities about the clip, with lights moving in the background, but Runco says the lights are likely to be stars.

Another clip, taken by Jones is simply “ice crystals or flakes of thruster residue in the near field are floating by, get hit by a thruster exhaust plume and zip out of the scene,” Jones said.

It’s one thing to believe that alien life is a statistical likelihood, and quite another to interpret lights in the sky as intergalactic contact. Check out the great article, and kudos to Jones and Runco for speaking out.

Spaceships on the Move!

Atlantis hitches a ride on a 747 back to KSC. Credit: NASA TV

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Atlantis has begun her journey back home to the Kennedy Space Center, hitching a ride on the Shuttle Carrier Aircraft, a modified Boeing 747. The flight took off at about 11:05 EDT on Monday morning from Edwards Air Force Base, and the duo will fly to Biggs Army Air Field in El Paso, Texas and spend the night there before resuming the cross-country trip on Tuesday. Of course, Atlantis just returned from space, landing at Edwards on May 24, concluding the STS-125 mission to service the Hubble Space Telescope for the last time. Track the flight here.

But Atlantis isn’t the only spacecraft on the move. The shuttle Endeavour just rolled around to launchpad 39A, after standing down from its potential rescue mission, (STS-400) in case Atlantis was unable to return home, and now is preparing for the STS-127, which will hopefully launch around June 13. Watch the video of the rollaround below. And the next missions to the Moon are now poised for launch.


On May 28, the Lunar Reconnaissaince Orbiter and the Lunar Crater Observation and Sensing Satellitespacecraft were transported to the launch pad. The transport of the stacked and encapsulated LRO/LCROSS payload began at about 2 am local time and culminated with the attachment of the payload atop the Atlas AV-20 rocket at about 9:30am.

LRO on the launchpad. Credit: NASA
LRO on the launchpad. Credit: NASA

The spacecraft will launch together June 17 from Cape Canaveral Air Force Station in Florida.

Using a suite of seven instruments, LRO will help identify safe landing sites for future human explorers, locate potential resources, characterize the radiation environment and test new technology. LCROSS will seek a definitive answer about the presence of water ice at the lunar poles. LCROSS will use the spent second stage Atlas Centaur rocket in an unprecedented way that will culminate with two spectacular impacts on the moon’s surface.

Learn more about LRO, and keep track of the countdown here.

Carnival of Space #105

Carnival 105. Credit: Ian O'Neill

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This week’s Carnival of Space is hosted by Ian O’Neill over at Discovery Space. Yes, Ian is at the Space Disco — if you’re confused, read this.

Click here to read the Carnival of Space #105

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, let Fraser know if you can be a host, and he’ll schedule you into the calendar.

Finally, if you run a space-related blog, please post a link to the Carnival of Space. Help us get the word out.

Astronomers Observe Formation of Largest Bound Structures in the Universe

The massive radio galaxy PKS 0745-191, for which the cluster is named, appears at the center of this Hubble Space Telescope image. The picture forms the inset in the Suzaku image above.

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An international team of astronomers has mapped the density and temperature of X-ray-emitting gas in the outskirts of a distant galaxy cluster.   The results, obtained with the orbiting Japanese X-ray telescope Suzaku, give the first complete X-ray view of a galaxy cluster, and provide insight into how such clusters come together.

“These Suzaku observations are exciting because we can finally see how these structures, the largest bound objects in the universe, grow even more massive,” said Matt George, the study’s lead author at the University of California, Berkeley.

The team trained Suzaku’s X-ray telescopes on the massive galaxy cluster PKS 0745-191, which lies 1.3 billion light-years away in the southern constellation Puppis.  Between May 11 and 14, 2007, Suzaku acquired five images of the million-degree gas that permeates the cluster.

The X-ray images of the cluster helped astronomers measure the temperature and density of the gas.  These provide clues about the gas pressure and cluster’s total mass.  The hottest, densest gas lies near the cluster’s center, while gas temperature and density steadily decline away from the center.

Astronomers believe the gas in the inner part of a galaxy cluster has settled into an ordered “relaxed” state in equilibrium with the cluster’s gravity.  But in the outer regions, where galaxies first begin a billion-year plunge towards the cluster’s center, the gas remains in a disordered state because it’s still falling inward.

“Clusters are the most massive, relaxed objects in the universe, and they are continuing to form now,” said team member Andy Fabian at the Cambridge Institute of Astronomy in the UK.

For the first time, this study shows X-ray emission and gas density and temperature out to the region where the gas is disordered, and where the cluster continues to assemble.

“It gives us the first complete X-ray view of a cluster of galaxies”, said Fabian.

This Suzaku image shows X-ray emission from hot gas throughout the galaxy cluster PKS 0745-191. Brighter colors indicate greater X-ray emission. The circle is 11.2 million light-years across and marks the region where cold gas is now entering the cluster. Inset: A Hubble optical image of the cluster's central galaxies is shown at the correct scale.
This Suzaku image shows X-ray emission from hot gas throughout the galaxy cluster PKS 0745-191. Brighter colors indicate greater X-ray emission. The circle is 11.2 million light-years across and marks the region where cold gas is now entering the cluster. Inset: A Hubble optical image of the cluster's central galaxies is shown at the correct scale.

In PKS 0745-191, the gas temperature peaks at 164 million degrees Fahrenheit (91 million C) about 1.1 million light-years from the cluster’s center. The temperature declines smoothly with distance, dropping to 45 million F (25 million C) more than 5.6 million light-years from the center.

To accurately measure X-ray emission at the cluster’s edge requires detectors with exceptionally low background noise.  Suzaku has advanced X-ray detectors, and it lies in a low-altitude orbit near the Earth’s magnetic field, which protects the observatory from energetic particles from the sun and beyond.

“With more Suzaku observations in the outskirts of other galaxy clusters, we’ll get a better picture of how these massive structures evolve,” added George.

Suzaku (Japanese for “red bird of the south”) was launched on July 10, 2005. The observatory was developed at the Japanese Institute of Space and Astronautical Science (ISAS), which is part of the Japan Aerospace Exploration Agency (JAXA), in collaboration with NASA and other Japanese and U.S. institutions.

The results were published in the May 11 edition of the Monthly Notices of the Royal Astronomical Society.

Source: NASA