Best Class Project Ever: 7th Graders Find a Cave on Mars

Sixteen seventh-graders at Evergreen Middle School in Cottonwood, Calif., found the Martian pit feature at the center of the superimposed red square in this image. Image Credit: NASA/JPL-Caltech/ASU

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Tip number one on “How to impress your classmates:” Find a mysterious cave on Mars. A group of 16 seventh-graders at Evergreen Middle School in Cottonwood, California, USA found a dark pit that appears to be an opening to a cave on Mars. Dennis Mitchell’s science class were examining Martian lava tubes as their project in the Mars Student Imaging Program offered by NASA and Arizona State University, which takes advantage of the huge database of images taken by the Mars Odyssey spacecraft. The students found the skylight pit on the slope of an equatorial volcano named Pavonis Mons, and it appears to be an entrance to an underground lava tube. Similar ‘cave skylight’ features have been found elsewhere on Mars, but this is the first seen on this volcano.

“The students developed a research project focused on finding the most common locations of lava tubes on Mars,” Mitchell said. “Do they occur most often near the summit of a volcano, on its flanks or the plains surrounding it?”

Mitchell said he and his students have been surprised how much interest there has been nation-wide in their discovery. “They were kind of shocked about the interest, and I think that they are just now starting to realize that they made a pretty neat discovery.”

The imaging program allows students in upper elementary grades through to college to participate in Mars research by having them develop a geological question to answer, and then directing the teams for the Mars-orbiting camera to take an image to answer their question. Since MSIP began in 2004, more than 50,000 students have participated.

Now, because of this find, the HiRISE high resolution camera on the Mars Reconnaissance Orbiter will take follow-up images of the pit to provide a better look at the object. HiRISE can image the surface at about 30 centimeters (12 inches) per pixel, which may allow a look inside the hole in the ground. This is part of the HiWISH program, where the public can submit suggestions to the science team for locations on Mars to the camera to image.

“It gives the students a good understanding of the way research is conducted and how that research can be important for the scientific community. This has been a wonderful experience,” Mitchell said.”

“Yeah it was a lot of fun because it wasn’t like any other science that we did, because we actually got to interact with real scientists instead of just people out of the book and stuff,” said 13-year-old Kody Rulofson, one of the students in Mitchell’s class.

Kody’s mother, Doni Rulofson said Kody and his twin brother Chase, also in the class, are inspired by the experience they had finding the cave. “They’re excited. They’re just beyond belief, they’re like, ‘we knew it was something really cool but we had no idea it was this much of an interest to NASA.'”

Odyssey has been orbiting the Red Planet since 2001, returning data and images of the Martian surface and providing relay communications service for Mars Rovers Spirit and Opportunity. Find out more about Odyssey here.

MRO has been in orbit since 2006, and has also amassed a huge database of images, which can be seen here.

Source: NASA

Israel Launches Spy Satellite

The launch of Israel's Ofeq 9 satellite with the Shavit launch vehicle on June 22, 2010. Image courtesy Israeli Aerospace Industries, Ltd.

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Israel launched an “Ofeq 9” satellite on Tuesday, an advanced remote sensing satellite that likely is capable of high resolution surveillance to monitor Iran’s nuclear program. The satellite was launched on Israel’s Shavit launch vehicle.

The Israel Defense Ministry gave no public details on the satellite, only releasing this statement following the launch: “A few minutes ago the State of Israel launched the Ofek-9 (Horizon-9) satellite from the Palmachim base (Israel’s Air Force test range). The results of the launch are being examined by the technical team.”

But in an Israel Defense Ministry document provided to Universe Today, the Ofeq 9 satellite was listed as capable of scanning a swath 7 km wide, with a resolution better than 70 cm and a pointing accuracy to within 20 meters. The satellite will initially be launched to an elliptical transfer orbit – 620 x 307 Km, and following the checkout, the final orbit will be approximately 500 km above Earth.

The Shavit launcher is a 3-stage launcher, 20 meters high and weighs approximately 30 tons.

With the launch of Ofeq-9, Israel has six spy satellites in space.

The satellite was made by Israel Aerospace Industries Ltd. The Shavit launcher has been in use since 1988, when the first Ofeq satellite was put into orbit.

Israel, which has the Middle East’s sole undeclared nuclear arsenal, regards Iran as its principal threat after repeated predictions by the Islamic republic’s hardline President Mahmoud Ahmadinejad of the Jewish state’s demise, according to news reports from Jerusalem. Israel suspects Iran of trying to develop atomic weapons under the guise of its nuclear program, a claim Tehran denies.

Sources: SpaceTravel.com, and special thanks to Avi Blizovsky, Editor Hayadan Science News in Israel.

Carnival of Space #159

This week’s Carnival of Space is hosted by Brian Wang over at Next Big Future.

Click here to read the Carnival of Space #159.

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.

Hubble Captures Beautiful Baby Stars

Hubble view of the huge star formation region N11 in the Large Magellanic Cloud. Credit: NASA, ESA and Jesús Maíz Apellániz (Instituto de Astrofísica de Andalucía, Spain).

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Within the Large Magellenic Cloud is one of the most active star forming regions in our nearby Universe. This new Hubble image highlights N11 – also known as the Bean Nebula — a beautiful region of energetic star formation. The billowing pink clouds that look like cotton candy and bright bubbles of glowing gasses and are telltale signs that stars are being created. Click the image for a larger, hi-res version.

Beans, bubbles and candy aren’t the only terrestrial shapes to be found in this spectacular image from the Hubble Space Telescope.

If you zoom into upper left (click this link for a zoom video) you’ll find a rose: The Rose Nebula LHA 120-N 11A. Its rose-like petals of gas and dust are illuminated from within, thanks to the radiation from the massive hot stars at its centre. N11A is relatively compact and dense and is the site of the most recent burst of star development in the region.

If you live in the southern hemisphere, both the Large Magellanic Cloud and its small companion, the Small Magellanic Cloud, are easily seen with the unaided eye. That’s a sight I would someday love to see!

For more videos and images of this region, see this ESA Hubble page.

John Glenn: Keep the Space Shuttles Flying

John Glenn
John Glenn flew on the space shuttle in 1998. Credit: NASA

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US spaceflight legend John Glenn has weighed in on the current human spaceflight debate, releasing an 8-page paper outlining his feelings and a potential plan to allow US astronauts to keep launching on US vehicles. While Glenn supports President Barack Obama’s plan to extend operations of the International Space Station and to forego returning to the Moon for the time being, he thinks retiring the space shuttles at this point is a mistake.

“The world’s only heavy lift spacecraft and the U.S.’s only access to space should stay in operation until suitably replaced by a new and well tested heavy lift vehicle,” Glenn wrote. “The Shuttle system is working extremely well, has had systems upgrades through the years, and has had “the bugs” worked out of it through many years of use. The Shuttle is probably the most complex vehicle ever assembled and flies in the harshest of environments. Why terminate a perfectly good system that has been made more safe and reliable through many years of development?”

But Glenn said the US also needs to develop heavy lift capability, and do it sooner rather than later. And while he supports the plan for NASA to contract with commercial companies to ferry astronauts and some cargo to and from the ISS, he also said NASA can’t rely solely on commercial space vehicles, which at present are unproven in their reliability.

Keeping the space shuttle program going would cost about $1 Billion a year. “That is a very small price to pay for maximizing the benefits from a $100 Billion national investment, and may even be cheaper than the final bill from the Russians,” Glenn said.

He blames NASA’s current predicament on Congress for not adequately funding the Constellation program.

He erred, however, in his statement that the “U.S. for the first time since the beginning of the Space Age will have no way to launch anyone into space – starting next January.” NASA did not launch humans into space from July 1975 to April 1981 – the end of Apollo and Skylab until the beginning of the shuttle era, as well as when spacecraft were grounded following the Apollo 1 fire in 1967, the Challenger accident in 1986 and the Columbia accident in 2003.

Glenn is the latest former astronaut to join the debate on NASA’s future and while some ex-astronauts are staunchly against cutting the Constellation program to return to the Moon, and others wholly endorse the plan, Glenn seemingly takes a middle ground.

Here are his suggested objectives:

Short Term
Extend the Shuttle. It is key to ISS ready access. Phase-in new space access providers only as they become experienced and have proven reliability.

Maximize research on the ISS – plan with the science community.

Use the ISS for long term Mars mission training.

Develop a fully tested replacement heavy-lift capability.

Long Term

Robotic exploration of Mars and other destinations such as asteroids.

Continue ISS research as long as it is making substantial contributions.

Increase preparation and planning for a Mars mission.

Determine – earth-to-Mars, or assembled-in-earth-orbit – to Mars.

Set a firm schedule –Go for Mars.

You can read Glenn’s full statement here.

This is not the first time Glenn has proposed to keep the shuttles flying. In 2008, he said “The shuttles may be old, but they’re still the most complex vehicles ever put together by people, and they’re still working very well,” he said after a Capitol Hill ceremony marking NASA’s 50th anniversary.

Gulf Oil Leak: Day 62 Update

Satellite image of the oil leak in the Gulf of Mexico, as seen on June 19, 2010. Credit: MODIS Rapid Response Team.

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Here’s the latest satellite image of the BP oil leak in the Gulf of Mexico. The oil keeps spreading towards the northeast, and appears as a maze of silvery-gray ribbons in this image from the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite. The MODIS team said that the spot of black just north of the location of the oil well may be smoke; reports from the National Oceanic and Atmospheric Administration say that oil and gas continue to be captured and burned as part of the emergency response efforts.

The MODIS team is putting out about two satellite images of the region a day, which can be seen at this link.

Below is a video from reporter David Hammer from the Times-Picayune newspaper in New Orleans, Louisiana, who is covering the BP oil spill, explaining the latest developments as of June 21,2010. Apologies for the 15 second ad at the beginning, but Hammer provides a good overview of what has been happening.

Oil spill video: Times-Picayune reporter update

Maybe ET’s Calling, But We Have the Wrong Phone

The search (xkcd)

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To date, SETI (Search for ExtraTerrestrial Intelligence) has focused on ETs who ‘phone home’ using the radio part of the electromagnetic spectrum, and even a very small region within that.

But what if ET’s phone doesn’t use radio waves? Sure the xkcd comic, is funny, but maybe it points to a deep flaw in our attempts to contact, or hear from, an ETI?

When Giuseppe Cocconi and Philip Morrison suggested the possibility of interstellar communication via electromagnetic waves in a 1959 paper in Nature, only radio was feasible, as we then had the ability to detect only artificial radio signals, if produced by ETIs with 1959 human technology. Since then we’ve developed the ability to detect a laser signal, brighter than the Sun (if only for a nanosecond) if it came from a source several light-years away … but lasers weren’t invented then.

What might ET’s equivalent of ants’ pheromones be?

Back in 1959 if you’d said that the Earth would, within a mere half century, started to go ‘radio quiet’, not many people would have taken you seriously. Yet that’s exactly what’s happened! Free to air (FTA) broadcasting, especially for TV, is being replaced by TV delivered over coaxial cable, optical fibers, or even the phone company’s twisted copper pairs. And where it’s continuing, as in satellite TV broadcasting, its power has dropped (today’s digital formats are more efficient than the old analog ones). Military radars, the brightest source of artificial radio waves by far, no longer broadcast in a single channel, but hop, rapidly, from frequency to frequency, to avoid jamming.

“Our improving technology is causing the Earth to become less visible,” says astronomer Frank Drake, SETI’s paterfamilias. “If we are the model for the universe, that is bad news.”

In the past half century SETI researchers have expanded the scope of their searches. Not only are far more radio channels being examined, but artificial signals in the optical are being sought too. How to decide which of the billions or trillions of possible radio channels to search? For example, the Allen Telescope Array will, when built, monitor a billion channels between 0.5 and 11 GHz – but that’s a trivial fraction of the entire radio waveband. Some ideas, however, seem cute; for example, the SETI Institute’s Gerald Harp has proposed searching at 4.462336275 gigahertz, in what’s called the PiHI range, because it’s the hydrogen atom’s emission frequency times pi. More seriously, Harvard University’s Paul Horowitz says optical SETI programs should really look at infrared frequencies “Stars are darker in the infrared and lasers are brighter and the smog goes away,” Horowitz says. Infrared allows astronomers to see into the galactic center, where dust scatters visible light.

There’s something rather ironic about SETI today; on the one hand, we recognize that our initial hopes were far too high, being based on overly simplistic assumptions; on the other, the tremendous progress in finding exoplanets has given us greater and greater certainty that Earth-like planets not only exist, but are, very likely, common. “All of astronomy has come to embrace this idea that there must be life out there,” says Harp.

So how to address the fact that we simply do not know what sorts of technologies a civilization like ours may have, a century or a millennium from now? After all, as Drake says “We are very conservative at SETI, we assume in our searches the existence of only things we ourselves have and know how to make.” Other scientists, and SETI enthusiasts, have proposed hunting in different electromagnetic realms, like gamma rays. Spacecraft that rely on nuclear fusion or antimatter-matter annihilation as a power source might produce such rays. But standard SETI strategy does not embrace such “speculative” scenarios.

SETI researchers, some say, should also contemplate what technologies supersmart aliens might possess and seek out the corresponding signals. In a 2008 arXiv paper, “Galactic Neutrino Communication“, John Learned of the University of Hawaii at Manoa suggested that ET could be sending beams of neutrinos Earth’s way. Energy requirements for such a beam make that scenario seem implausible, but not necessarily impossible. Detectors currently under construction, such as IceCube at the South Pole, could spot unexpected stray neutrinos. If a few with the same energy came from the same direction, astronomers would know something screwy was up.

In another paper, “The Cepheid Galactic Internet“, Learned suggests that ET could send a signal using a neutrino beam to deliver energy to a Cepheid variable. A Cepheid “blows up and comes crashing back down,” he says. “And the energy builds up and it blows again, like a geyser.” ET could leverage a Cepheid’s inherent instability by delivering a boost of energy that messes with the star’s schedule. Looking through existing data could reveal whether such meddling has occurred. “All that is needed is people analyzing for other reasons to do their analyses in another way,” Learned says.

Drake and most others agree that SETI’s approach should be multidirectional – let a thousand alien hunters bloom. The only ideas that don’t do anybody any good, Horowitz says, are the ones for which there is no conceivable way to look. “I’d like to keep an open mind,” he says, “but not so much that my brain falls out.”

Physicist Paul Davies of Arizona State University in Tempe, however, suggests that researchers don’t need to know what to look for. Find the fishy thing first, and then argue about its origin, he says.

As Davies has argued, maybe discovering ET does indeed depend on a thought revolution. Fifty years of signal-less searching suggests that the problem could lie not with the aliens among the stars, but with ourselves.

Maybe the sentient ants should not give up, just yet.

Sources: Science News. Cocconi and Morrison’s 1959 Nature paper (copyright Nature)

Titan + Dione = New Desktop

Titan and Dione as seen by Cassini. Credit: NASA/JPL/Space Science Institute

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Another stunning image from the Cassini spacecraft, suitable for wallpaper on your desktop. Click image for larger version, or click here for a large 1.125 MB version.

This is Saturn’s moon Dione, in crisp detail, against a hazy, ghostly Titan. Simply stunning.

The “wispy” terrain on Dione is visible, and on Titan are hints of atmospheric banding around Titan’s north pole. This view looks toward the Saturn-facing hemisphere of Dione (1123 kilometers, 698 miles across) and Titan (5150 kilometers, 3200 miles across), and was taken on April 10, 2010.

No images available yet from Cassini’s extremely close flyby of Titan over the weekend where it buzzed the hazy moon at an altitude of just 880 kilometers (547 miles) above the surface.

That is 70 kilometers (43 miles) lower than it has ever been at Titan before. The reason for attempting such a close pass is to try and establish if Titan has a magnetic field of its own. But the Cassini team went through hours and hours of calculations for this close flyby, as Titan’s atmosphere applies torque to objects flying through it, much the same way the flow of air would wiggle your hand around if you stuck it outside a moving car window. According to the Cassini website, when engineers calculated the most stable and safe angle for the spacecraft to fly, they found it was almost the same as the angle that would enable Cassini to point its high-gain antenna to Earth. So they cocked the spacecraft a fraction of a degree, enabling them to track the spacecraft in real-time during its closest approach. They set up the trajectory with thrusters firing throughout the flyby to maintain pointing automatically.

The images and data gathered should be amazing, as if everything went as planned, the flyby ended with the ultra violet imaging spectrograph (UVIS) instrument capturing a stellar occultation outbound from Titan. We’ll keep you posted!

Source: CICLOPS, Carolyn Porco on Twitter

Stunning Sunrise and Aurora, As Seen from the Space Station

Sunrise as seen by Doug Wheelock (Astro_Wheels on Twitter) from the ISS.

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Expedition 23 astronaut Soichi Noguchi took and shared so many amazing images during his 6-month stay on board the International Space Station, and I was a little worried that his return to Earth would result in a bit of a let-down in the space imaging department. I now see I had nothing to fear: Three new members of the Expedition 24 crew arrived at the ISS late last week and Doug Wheelock seems to have filled Soichi’s shoes (or socks, since they don’t wear shoes on the ISS) quite nicely. He posted two new images today on his Twitpic page that are nothing short of stunning. This image, above of an orbital sunrise provides a great look at the ISS bathed in “morning” light.

“A stunning sunrise aboard the International Space Station, as seen from the Russian MRM1 Module. We’re blessed with 16 sunrises each day!” Wheelock, a.k.a Astro_Wheels wrote.

See below for an aurora he captured over the South Pole.

An aurora seen over the South Pole, from the ISS. Credit: Doug Wheelock, NASA.

“A breath-taking masterpiece being painted in the sky over the South Pole. ‘The Southern Lights’…like brush strokes from the Master’s hand…” wrote Wheelock.

Follow Wheelock on Twitter to get the latest images he takes during his Expedition.

A recent image of a sunset taken from the ISS, is also incredibly beautiful. It wasn’t taken by Wheelock, but made NASA’s Earth Observatory’s website “Image of the Day” feature. Marvelous! The NASA page doesn’t say which astronaut took the image. Click the image for a larger, non-annotated view.

Sunset from the ISS shows the different layers of the atmosphere. Credit: NASA

And here’s a video I found of an orbital sunrise taken in 2006 on the STS-116 space shuttle mission.

Astronomy Without A Telescope – SETI 2.0

Allen Telescope Array. Credit: SETI Institute

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Fifty years of eerie silence in the search for extra-terrestrial intelligence has prompted some rethinking about what we should be looking for.

After all, it’s unlikely that many civilizations would invest a lot of time and resources into broadcasting a Yoo-hoo, over here signal, so maybe we have to look for incidental signs of alien activity – anything from atmospheric pollution on an exoplanet to signs of stellar engineering undertaken by an alien civilization working to keep their aging star from turning into a red giant.

We know a spectroscopic analysis of Earth’s atmosphere will indicate free molecular oxygen – a tell tale sign of life. The presence of chlorofluorocarbons would also be highly suggestive of advanced industrial activity. We also know that atomic bomb tests in the fifties produced perturbations to the Van Allen belts that probably persisted for weeks after each blast.

These are planet level signs of a civilization still below the level of a Kardashev Type 1 civilization. We are at level 0.73 apparently. A civilization that has reached the Type 1 level is capable of harnessing all the power available upon a single planet – and might be one that inadvertently signals its presence after thoughtfully disposing of large quantities of nuclear waste in its star. To find them, we should be scanning A and F type stars for spectral signatures of technetium – or perhaps an overabundance of praseodymium and neodymium.

We might also look for signs of stellar engineering indicative of a civilization approaching the Kardashev Type 2 level, which is a civilization able to harness all the power of a star. Here, we might find an alien civilization in the process of star lifting, where an artificial equatorial ring of electric current creates a magnetic field sufficient to both increase and deflect all the star’s stellar wind into two narrow polar jets.

Left image - A proposed model for 'star lifting'. An artificial equatorial ring of electric current (RC) produces a magnetic field which enhances and directs the star's stellar wind though magnetic nozzles (MN) to produce two polar jets (J). Right image (Credit: SETI institute) - Artists impression of the completed Allen Telescope Array for future SETI observations. The lead image for this article is part of the current Allen Array prototype, comprising 42 of the proposed 350 dishes.

These jets could be used for power generation, but might also represent a way to prolong the life of an aging star. Indeed, this may become a vital strategy for us to prolong the solar system’s habitable zone at Earth’s orbit. In less than a billion years, Earth’s oceans are expected to evaporate due to the Sun’s steadily increasing luminosity, but some carefully managed star lifting to modify the Sun’s mass could extend this time limit significantly.

It’s also likely that Type 2 civilizations will play with Hertzsprung–Russell (H-R) parameters to keep their Sun from evolving onto the red giant branch of the H-R diagram – or otherwise from going supernova. Some well placed and appropriately shielded nuclear bombs might be sufficient to stir up stellar material that would delay a star’s shift to core helium fusion – or otherwise to core collapse.

It’s been hypothesized that mysterious giant blue straggler stars, which have not gone supernova like most stars of their type would, may have been tinkered with in this manner (some stress on the word hypothesized there).

As for detecting Type 3 civilizations… tricky. It’s speculated that they might build Dyson nets around supermassive black holes to harvest energy at a galactic level. But indications are that they then just use all that energy to go around annoying the starship captains of Type I civilizations. So, maybe we need to draw a line about who exactly we want to find out there.

Further reading:

Starry Messages: Searching for Signatures of Interstellar Archaeology http://arxiv.org/abs/1001.5455

Detectability of Extraterrestrial Technological Activities http://www.coseti.org/lemarch1.htm