More Researchers Say Liquid Water Present on Mars Now

Blobs of something "growing" on the Phoenix lander's legs.

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Finding perchlorates on Mars was not only surprising for the Phoenix lander science team, it also has created a bit of a rift among the researchers. In March, Ian reported on one scientist who used strictly photographic evidence to say that blobs appearing on the lander’s legs were actually water. Other scientists, however, including principal investigator Peter Smith were dubious about the “water on Mars now” claims. But now, a group of researchers at the University of Arkansas say they have now demonstrated a potential stable liquid on present-day Mars in the immediate environment of the lander.

The salts formed from perchlorates discovered at the Phoenix landing site act as “anti-freeze” and have the potential to be found in a liquid solution under the temperature and pressure conditions on present-day Mars, say professor Vincent F. Chevrier and graduate students Jennifer Hanley and Travis S. Altheide. Their research is published in the current issue of Geophysical Research Letters.

“Under real, observed Martian conditions, you can have a stable liquid,” said Chevrier.

The researchers studied the properties of sodium and magnesium perchlorates, salts detected by the Phoenix lander, under the temperature, pressure and humidity conditions found at the landing site. The discovery of perchlorates on Mars by the Phoenix mission surprised scientists – the compounds are rare on Earth, found mostly in extremely arid environments such as the Atacama Desert in Chile.

This image was taken by the Phoenix land on the 97th day of the mission.  Credit: NASA/JPL
This image was taken by the Phoenix land on the 97th day of the mission. Credit: NASA/JPL


The scientists studied the properties of these salts at varying temperatures using the Andromeda Chamber in the W.M. Keck Laboratory for Space Simulation – a chamber that can imitate the pressure and atmospheric conditions found on Mars. They also performed thermodynamic calculations to determine the state of salt and water combinations on the Martian surface and to see if there was any potential for liquid to be found.

The extreme temperatures found on Mars typically lead to either crystallization or evaporation of water, making it difficult to imagine that water could be found in liquid form. However, salts have been shown to lower the freezing point of water – which is why street crews use salt on the roads to melt ice, Hanley said. Some salts, like perchlorates, lower the freezing point substantially. It turns out that the temperature for the liquid phase of magnesium perchlorate – 206 degrees Kelvin – is a temperature found on Mars at the Phoenix landing site. Based on temperature findings from the Phoenix lander, conditions would allow this perchlorate solution to be present in liquid form for a few hours each day during the summer.

“The window for liquid is very small,” Hanley said. Nevertheless, this finding further supports the possibility of finding life on Mars.

“You don’t necessarily need to have a lot of water to have life,” Chevrier said. “But you need liquid water at some point.”

Source: University of Arkansas

New Technique Could Find Another “Pale Blue Dot”

EPOXI image of the Moon transiting Earth from 31 million miles. Credit: NASA/JPL

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By looking back at Earth from alien’s point of view, scientists have developed a new technique to look for other worlds that might harbor oceans, and therefore life. Using the old Deep Impact spacecraft, which is now being used for the EPOXI mission, scientists are able to look at the spectrum of an extrasolar planet’s light which would reveal the presence of water. “We used the High Resolution Imager telescope on Deep Impact to look at Earth from tens of millions of miles away,” said Nicolas B. Cowan, of the University of Washington, ” and developed a method to indicate the presence of oceans by analyzing how Earth’s light changes as the planet rotates. This method can be used to identify extrasolar ocean-bearing Earths.”

Last year, the EPOXI science team was able to take videos of the Moon transiting Earth, (see our article from July 2008). The team has now practiced the technique by looking back at Earth, and have determined that they should be able to detect oceans on other worlds by looking at the changing spectrum of light the planet gives off as it rotates.

Cowan is lead author of a paper on this research appearing in the August 2009 issue of the Astrophysical Journal. Our planet looks blue all the time because of Rayleigh scattering of sunlight by the atmosphere, the same reason that the sky appears blue to us down on the surface, points out Cowan. “What we studied in this paper was how that blue color changes in time: oceans are bluer than continents, which appear red or orange because land is most reflective at red and near-infrared wavelengths of light. Oceans only reflect much at blue (short) wavelengths,” said Cowan.

“A ‘pale blue dot‘ is the best picture we will get of an Earth-like extrasolar world using even the most advanced telescopes planned for the next couple decades,” Cowan continued. “So how do we find out if it is capable of supporting life? If we can determine that the planet has oceans of liquid water, it greatly increases the likelihood that it supports life.”

palebluedot_jpg This narrow-angle color image of the Earth, dubbed ‘Pale Blue Dot‘, is a part of the first ever ‘portrait’ of the solar system taken by Voyager 1, and made famous by astronomer Carl Sagan. The spacecraft acquired a total of 60 frames for a mosaic of the solar system from a distance of more than 4 billion miles from Earth and about 32 degrees above the ecliptic. From Voyager’s great distance Earth is a mere point of light, less than the size of a picture element even in the narrow-angle camera. Earth was a crescent only 0.12 pixel in size. Coincidentally, Earth lies right in the center of one of the scattered light rays resulting from taking the image so close to the sun. This blown-up image of the Earth was taken through three color filters — violet, blue and green — and recombined to produce the color image. The background features in the image are artifacts resulting from the magnification. Credit: NASA JPL

The maps that the team created are only sensitive to the longitudinal (East – West) positions of oceans and continents. Furthermore, the observations only pick out what is going on near the equator of Earth: the equator gets more sunlight than higher latitudes, and the EPOXI spacecraft was above the equator when the observations were taken. These limitations of viewing geometry could plague observations of extrasolar planets as well: “We could erroneously see the planet as a desert world if it had a nearly solid band of continents around its equator and oceans at its poles,” said Cowan.

Other things besides water can make a planet appear blue; for example, in our solar system the planet Neptune is blue due in part to the presence of methane in its upper atmosphere. “However, a Neptune-like world would appear as an unchanging blue using this technique, and again it’s the changes in the blue color that reveal oceans to us,” said Cowan. “There are some weird scenarios you can dream up that don’t involve oceans but would lead to varying patches of blue on a planet, but these are not very plausible.”

“A spectrum of the planet’s light that reveals the presence of water is necessary to confirm the existence of oceans,” said Drake Deming, a co-author of the paper at NASA’s Goddard Space Flight Center in Greenbelt, Md. Instruments that produce a spectrum are attached to telescopes and spread out light into its component colors, like a prism separates white light into a rainbow. Every element and molecule emits and absorbs light at specific colors. These colors can be used like a fingerprint to identify them.

“Finding the water molecule in the spectrum of an extrasolar planet would indicate that there is water vapor in its atmosphere, making it likely that the blue patches we were seeing as it rotates were indeed oceans of liquid water. However, it will take future large space telescopes to get a precise spectrum of such distant planets, while our technique can be used now as an indication that they could have oceans,” said Deming. The technique only requires relatively crude spectra to get the intensity of light over broad color ranges, according to the team.

EPOXI is a combination of the names for the two extended mission components: a search for extrasolar planets during the cruise to Hartley 2, called Extrasolar Planet Observations and Characterization (EPOCh), and the flyby of comet Hartley 2, called the Deep Impact eXtended Investigation (DIXI).

Source: NASA

Discovery Discovers Ian O’Neill

Ian O'Neill

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You might have heard through the celestial grape vine that Universe Today correspondent Ian O’Neill has been tagged to lead the space news team over at the Discovery Channel’s space blog network. So if you’re wondering why there aren’t many O’Neill articles over here, or at his own website Astroengine.com, that’s because he writing (and editing) his big heart over at Discovery.com: Space Disco. The previous producer, Dave Mosher has moved on to manage the web development for a non-profit foundation.

A big thanks to Ian for all his dedicated work on Universe Today and I really hope everything goes well with his work over at the Discovery Channel.

Ian has promised he’ll still be contributing the occasional article for Universe Today. And if he’s too busy for that, we’ll still be linking to his coverage when we can.

So congrats Ian!

Lava Viscosity

A'a lava

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When it comes to liquids, viscosity is a measurement of how thick or syrupy it is. Water has low viscosity, while corn syrup, for example, is highly viscous. You can measure lava in terms of viscosity as well. And the lava viscosity defines the size and shape of a volcano. Even though lava is 100,000 times more viscous than water, it can still flow great distances.

When lava has low viscosity, it can flow very easily over long distances. This creates the classic rivers of lava, with channels, puddles and fountains. You can also get bubbles of lava filled with volcanic gasses that burble and pop on the surface of the lava. And over time, volcanoes made from low lava viscosity are wide and have a shallow slope; these are known as shield volcanoes. Classic examples of shield volcanoes are Mauna Kea and Mauna Loa in Hawaii, as well as Olympus Mons on Mars.

When lava has a high viscosity, it’s very thick and doesn’t flow very well at all. Instead of rivers of lava, you can get crumbling piles of rock flowing down hill. It can also clog up the volcanic vent and form blocks that resist the flow of lava. Viscous lava will trap pockets of gas within the rock, and not let them pop as bubbles on the surface. But most importantly, highly viscous lava is associated with explosive eruptions and dangerous pyroclastic flows.

An example of a low viscosity (fast flowing) lava is basaltic lava. This flows quickly out of a volcano at a temperature of about 950 degrees Celsius. This flows out for great distances creating shield volcanoes or flood basalt fields. An example of high viscosity lava is felsic lava, like rhyolite or dacite. It erupts at lower temperatures, and can flow for tens of kilometers.

We have written many articles about lava for Universe Today. Here’s an article about lava flows, and here’s an article about the temperature 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.

Volcanic Tuff

Welded tuff at Yellowstone National Park.

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When volcanoes erupt, they can blast out lava, hot gasses, rocks and clouds of ash. Some of this ash rises up into the air and can travel for hundreds of kilometers in the air. Other ash pours down the sides of the volcano in great pyroclastic flows. When this ash cools, hardens and forms rocks, this material is called volcano tuff.

Geologists have a catch all name for rock ejected out of a volcano during an eruption: tephra. That can include tiny ash particles or large rocks. Particles smaller than 2 mm in diameter are considered ash. And when this ash is compacted down into rock, then you get volcanic tuff.

Tuff can range in texture, chemistry and mineral properties. Some tuff is very soft and can be easily dug with hand tools. Other tuff has been keep under pressure and cemented together to the point that it’s as hard as obsidian. Since there’s always been volcanism on Earth, volcanic tuff can be found around the Earth, in many different places and rock layers. Some is exposed on the surface, while others are buried by other eruptions or eroded material.

One of the most dramatic events is a “nuee ardente”. This is a glowing avalanche of hot ash cascading down the side of a volcano at speeds greater than 100 km/hour. When the ash avalanche comes to a stop, all this ejecta will compact together to form welded tuffs. There are large regions like this in Yellowstone National Park.

Ancient people used the soft nature of volcanic tuff to make buildings. They could carve out bricks from the soft rock to make walls.

We have written many articles about volcanoes for Universe Today. Here’s an article about volcanic ash, and here’s an article about volcanic rock.

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.

Carnival of Space #104

A new Carnival of Space is now available. This week, #104 is hosted over at Mang’s Bat Page.

Click here to read the Carnival of Space #104.

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.

What is a Volcano Conduit?

Steins Pillar, a hardened volcano conduit.

When a volcano erupts, it’s spewing forth lava, ash and hot rock. But where does this material come from, and how does it get to the surface? A volcano conduit is the pipe or vent at the heart of a volcano where material wells up from beneath the surface.

The surface of the Earth is relatively cool, but things get hotter as you descend beneath the ground. When you get about 30 km down (beneath the continents), you reach the Earth’s mantle. This is region of the Earth where rocks can be heated to more than 1,000 degrees C. Because of this high heat and pressure, liquid rock squeezes out of the mantle and collects in magma chambers beneath the Earth’s crust. The magma is “lighter” than the surrounding rock, so it floats to the surface, finding its way though cracks and faults in the crust. Eventually it reaches the surface and erupts as a volcano.

The volcano conduit is the pipe that carries this magma from the magma chamber, up through the crust and through the volcano itself until it reaches the surface. Stratovolcanoes, the largest kind of volcano, can have entire networks of volcano conduits inside them, and they can have eruptions from the central crater at the top, or from volcanic vents on the side.

After an eruption, the lava can cool and harden in the volcano conduit forming a hard plug. In some cases the plug causes the volcano to build up additional pressure and have an explosive eruption. In other cases, the volcano goes extinct, and the hard plug is all that remains when the rest of the volcano erodes away. Some of the most beautiful natural structures are these volcanic necks perching up above the surroundings.

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.

Mount Etna

Mount Etna seen from space. Image credit: NASA

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Mount Etna is a stratovolcano on the east side of the Island of Sicily. Standing 3,329 meters tall, Etna is the second largest volcano in Europe, and the highest mountain in Italy south of the Alps. But more importantly, Mount Etna is one of the most active volcanoes in the world, in an almost constant state of eruption.

Etna is classified as a stratovolcano (also known as a composite volcano). This is where many different kinds of eruptions over time have built up the huge mountain. You can have layers of lava, rock and ash, and many volcanic vents reaching the surface and capable of erupting. Many of the largest, most dangerous volcanoes in the world are stratovolcanoes (Mount St. Helens, for example).

Geologists believe the Etna started erupting about 300,000 years ago. In the last 35,000 years or so the mountain has had many explosive eruptions with pyroclastic flows cascading down its banks. Ash from Mount Etna eruptions has been found in Rome, located 800 km away. The successive eruptions have also caused calderas on the mountain to collapse creating depressions. There are now almost constant eruptions on Etna, with severe eruptions happening every 20 years or so.

You would think that the Italians would be nervous about having an active volcano in their back yard, but people actually live on the slopes of Etna. There are vineyards and orchards spread across its flanks; that’s because the rich volcanic soil is so good for planting. For example, in 2007 an eruption brought rivers of lava flowing down the slopes of Etna into an uninhabited valley. Villagers in the city of Catania on the island of Sicily could watch the eruption. Only an airport was closed during the eruption.

We have written many articles about Mount Etna for Universe Today. Here’s an article about images of Etna captured by 4 different satellites. And here’s an article about Mount Saint Helens.

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.

Vulcan and Volcanoes

Statue of Vulcan. Image credit: Marie-Lan Nguyen

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The name “volcano” comes the island of Vulcano, located in the Mediterranean Sea off the coast of Sicily. The Romans believed that Volcano was the chimney to the god Vulcan’s workshop. The island itself was thought to come from the debris that came out of the god’s furnace. The Romans believed that the earthquakes that shook the ground around the island came from Vulcan working in his shop, creating weapons for the gods to make war on one another.

The volcanic activity on the island of Vulcano comes from the northward motion of the African Plate colliding with the Eurasian Plate. This has opened up three volcanic hotspots on the island. There are two old stratovolcano cones at the southern end of the island, and then the most active Fossa cone in the center, and another at the north of the island. Currently about 470 people live on the island of Vulcano, getting their income from tourism.

In mythology, Vulcan was married to Venus, the goddess of love and beauty. The Romans believed that eruptions on Mount Etna in Sicily were caused by Vulcan’s anger at Venus. He works the forge so angrily that the metal turns red hot and sparks and smoke erupt from the top of the volcano.

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

UT Briefs: Shuttle Lands, Re-living Phoenix

Atlantis touches down in California. Credit: NASA

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Space Shuttle Lands

Space shuttle Atlantis landed safely in California on Sunday morning after “dynamic and unpredictable” weather kept the orbiter from returning to Florida. Atlantis touched down on runway 22 of Edwards Air Force Base at 11:39 am EDT (1539 GMT) Sunday, the first of two opportunities to land the shuttle in California. Atlantis spent nearly 13 days in orbit on the STS-125 mission, successfully repairing and upgrading the Hubble Space Telescope during a series of five spacewalks. Atlantis will be ferried to Kennedy Space Center on top of a modified 747 in about a week. Next shuttle mission: STS-127, slated for liftoff on June 13, on a trip to the International Space Station.


Remembering Phoenix

Do you remember what you were doing a year ago? You may recall the Phoenix Mars lander touched down on the Red Planet a year ago, and if you were on Twitter back then, you could follow the spacecraft’s progress via the fledgling social networking device. The “voice” of Phoenix’s Twitter account, Veronica McGregor, is re-living the events of a year ago by re-posting her “Tweets” in real time as they were written a year ago. It is a fun way to stroll down memory lane.