Tethys Floating Past Saturn

Tethys floating past the massive golden globe of Saturn. Image credit: NASA/JPL/SSI Click to enlarge
Tethys floats before the massive, golden-hued globe of Saturn in this natural color view. The thin, dark line of the rings curves around the horizon at top.

Visible on Tethys (1,071 kilometers, or 665 miles across) are the craters Odysseus (top) and Melanthius (bottom). The view looks toward the anti-Saturn side of Tethys.

Images taken using red, green and blue spectral filters were combined to create this color view. Tethys is apparently darker than Saturn at these wavelengths. The edge of the planet appears fuzzy, which may indicate that we are seeing haze layers that are separated from the main cloud deck.

The images were acquired by the Cassini spacecraft narrow-angle camera on Dec. 3, 2005, at a distance of approximately 2.5 million kilometers (1.6 million miles) from Saturn. The image scale is 15 kilometers (9 miles) per pixel on Saturn and 13 kilometers (8 miles) per pixel on Tethys.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org .

Original Source: NASA/JPL/SSI News Release.

Pluto is Colder Than Charon

Pluto & Charon viewed from the surface of one of Pluto’s newly discovered candidate satellites. Image credit: David A. Aguilar (CfA). Click to enlarge
Mercury is boiling. Mars is freezing. The Earth is just right. When it comes to the temperatures of the planets, it makes sense that they should get colder the farther away they are from the Sun. But then there is Pluto. It has been suspected that this remote world might be even colder than it should be. Smithsonian scientists now have shown this to be true.

Scientists continue to discuss whether Pluto is a planet or should be considered a refugee from the Kuiper belt. Whatever its classification, Pluto and its moon Charon are certain to harbor secrets about the early history of planet formation. Charon is roughly half the diameter of the planet itself, and they form a unique pair in our solar system. How they came to be together remains a mystery.

Located thirty times farther away from the Sun than the Earth, sunlight reaching the surface of Pluto is feeble at best, with daytime resembling dark twilight here at home. Pluto’s temperature varies widely during the course of its orbit since Pluto can be as close to the sun as 30 astronomical units (AU) and as far away as 50 AU. (An AU is the average Earth-Sun distance of 93 million miles.) As Pluto moves away from the Sun, its thin atmosphere is expected to freeze and fall to the surface as ice.

Reflected sunlight gathered with instruments such as the Keck telescope in Hawaii and the Hubble Space Telescope suggested the surface of Pluto might be colder than it should be, unlike Charon’s. However, no telescope capable of directly measuring their thermal emission (their heat) was able to peer finely enough to distinguish the two bodies. Their close proximity presented a formidable challenge since they are never farther apart than 0.9 arcseconds, about the length of a pencil seen from 30 miles away.

Now, for the first time, Smithsonian astronomers using the Submillimeter Array (SMA) on Mauna Kea in Hawaii have taken direct measurements of thermal heat from both worlds and found that Pluto is indeed colder than expected, colder even than Charon.

“We all know about Venus and its runaway greenhouse effect,” said Mark Gurwell of the Harvard-Smithsonian Center for Astrophysics (CfA), co-author on this study along with Bryan Butler of the National Radio Astronomy Observatory. “Pluto is a dynamic example of what we might call an anti-greenhouse effect. Nature likes to leave us with mysteries – and this was a big one.”

During the observations, the SMA utilized its most extended configuration to obtain high-resolution interferometric data, allowing separate “thermometer” readings for Pluto and Charon. It found that the temperature of the ice-covered surface of Pluto was about 43 K (-382 degrees F) instead of the expected 53 K (-364 degrees F), as on nearby Charon. This fits the current model that the low temperature of Pluto is caused by equilibrium between the surface ice and its thin nitrogen atmosphere, not just with the incoming solar radiation. Sunlight (energy) reaching the surface of Pluto is used to convert some of the nitrogen ice to gas, rather than heat the surface. This is similar to the way evaporation of a liquid can cool a surface, such as sweat cooling your skin.

“These results are really exciting and fun as well,” said Gurwell. “Imagine taking something’s temperature from almost three billion miles away without making a house call!”

This research will be presented at the 207th meeting of the American Astronomical Society in Washington, DC.

Headquartered in Cambridge, Mass., the Harvard-Smithsonian Center for Astrophysics (CfA) is a joint collaboration between the Smithsonian Astrophysical Observatory and the Harvard College Observatory. CfA scientists, organized into six research divisions, study the origin, evolution and ultimate fate of the universe.

Original Source: CfA News Release

Podcast: Gravity Tractor Beam for Asteroids

Forget about nuclear weapons, if you need to move a dangerous asteroid, you should use a tractor beam. Think that’s just Star Trek science? Think again. A team of NASA astronauts have recently published a paper in the Journal Nature. They’re proposing an interesting strategy that would use the gravity of an ion-powered spacecraft parked beside an asteroid to slowly shift it out of a hazardous orbit. Dr. Stanley G. Love is member of the team and speaks to me from his office in Houston.
Continue reading “Podcast: Gravity Tractor Beam for Asteroids”

Podcast: Gravity Tractor Beam for Asteroids

Asteroid 951 Gaspra taken by the Galileo spacecraft. Image credit: NASA/JPL. Click to enlarge.
Listen to the interview: Gravity Tractor Beam (4.8 MB)

Or subscribe to the Podcast: universetoday.com/audio.xml

Fraser Cain: Dealing with asteroids that are going to hit the Earth, now as I understand it, you need to find a crew of top quality oil miners. And you need to put them on the Space Shuttle and send them with a bunch of nuclear bombs to the asteroid to blow it up. Now you’re telling me that maybe this isn’t the best way?

Dr. Stanley G. Love: Well, it depends on what your goal is. If your goal is to make a movie that’s going to make a ton of money, then go wild; that’s exactly the right way to do it. If your goal is to actually prevent an impact with the Earth, though, we’re hoping there might be a simpler method of dealing with this.

Fraser: All right, so what’s the simpler method that you’re suggesting?

Love: Well, the method that we’re suggesting is to send a relatively large and heavy spacecraft – not so large and heavy that we can’t imagine it – to the asteroid, and instead of trying to blow up the asteroid, or land on it and push the thing aside (both of those ideas have been suggested, but they have some difficulties), we’re suggesting you just park the spacecraft next to it and let it hover there. And if you let it hover there for something like a year, very very gradually, the tiny gravitational pull between the asteroid and the spacecraft is going to pull the asteroid over in the direction of the spacecraft. The spacecraft is hovering in a constant distance from the asteroid, and what this means is that it’s very gradually pulling the asteroid off course using gravity as sort of a tow line. And if you can get enough warning on your asteroid – if you know it’s coming 20 years or so before it’s going to hit – then you can get the spacecraft out there and have it pull for about a year, you can pull it enough so that instead of hitting the Earth, it will miss the Earth.

Fraser: Now all the media, and all of those disaster movies revolve around some astronomer spotting a dangerous asteroid three months before it’s going to hit. It sounds like your solution is more in the 20 year range. Do you think that’s the more realistic scenario now these days?

Love: It’s hard to know. We haven’t really discovered all of the asteroids that could potentially hit the Earth yet. We’ve got a lot of people very busily working on that problem; there are searches going on every night. I think a lot of them are automated, and not some lonely guy on a mountaintop with his eye to the lens of a telescope there. And it is possible that tomorrow we could realize that there’s something coming that could hit us that we didn’t know about and it could be three months away from impacting the Earth. That would be certainly unfortunate. But in the future we are likely to know all these things; know all their orbits, and we can predict a hit long before it’s going to hit us. And that’s the sort of scenario that our solution will be able to deal with.

Fraser: And so what size of asteroids would you be able to deal with?

Love: A couple hundred metres in size. So the size of a football stadium or convention center.

Fraser: And what would the spacecraft itself look like? What kind of components would it have on it?

Love: When we came up with the idea for our little paper, we pulled a spacecraft design essentially off the shelf. It’s NASA’s Prometheus project, where they were going to send a large nuclear powered spacecraft to orbit Jupiter’s moon Europa, and do a lot of interesting science there. It’s a 20-ton spacecraft with electric thrusters, that is it uses electric power to heat a gas to extremely high temperatures and squirt it out the back. You get marvelous fuel economy; a lot of ability to move a spacecraft with a small amount of fuel, but the thrust is really low. You can only get a newton, or so (a fifth of a pound) of force. So you have a large electric propulsion, nuclear powered spacecraft – this is probably going to be a long skinny thing, because you’ll need a lot of radiators to reject the waste heat from the nuclear reactor. It’s going to have a set of thrusters, a fuel tank, and some guidance and navigation components. Depending on how you set this spacecraft up, we decided that if you put the reactor, which is heavy, and the fuel tank, which is heavy, down close to the asteroid – hanging from the thrusters – then you get more mass close to the asteroid, and that increases your gravitational pull as gravitational pull decreases rapidly as you increase the distance between the two masses. And it also helps stabilize your spacecraft and just helps you all around if you put your heavy components hanging down by the asteroid with the thrusters up at the top.

Fraser: Oh, I see, it would almost be if you had a ball at the end of a rope, hanging down with the heavy part – the reactor and all the fuel – hanging as close to the asteroid as you can, while all the thrusters are further up the rope pulling it away.

Love: That’s exactly right. Of course you need to tip your thrusters out away so the plume of hot gas coming out of them doesn’t hit the asteroid. It does no good trying to pull an asteroid closer to you with gravity and at the same time that you are pushing at it with your thruster plumes. So you need those outward so the plumes miss the asteroid and that will help improve your towing force.

Fraser: Now do you have any targets that you think might be a good victim of this kind of movement strategy?

Love: We were sort of developing the idea as a generic idea, and fly to anything. However, there’s Asteroid 99942 Apophis which is supposed to make a close pass of the Earth I think in 2029. And if that asteroid happens to pass through exactly the right point in space as it goes past the Earth, it has a chance to come back in 7-8 years and hit us, which would be bad. And that asteroid is an excellent target for this kind of a mission. If we can get to it before that first Earth flyby, that would line it up for impact the second time around. And the reason for that is that these flybys warp the path of the asteroid so that a tiny tiny change in the flight direction before the flyby gives a huge change in the flight direction after the flyby. So it’s like a bank shot in pool. A little tiny mistake on the first part, after the bounce, the mistake gets multiplied. So you could use a gravitational tractor that wasn’t nuclear powered and didn’t weight 20 tons. You could use a 1-ton, chemical-propelled gravity tractor to pull this asteroid just slightly off course before that Earth flyby so the asteroid is going no where near us.

Fraser: I see, if you have an asteroid that coming towards us 20 years out, you could move your big ion engine-powered tractor. How long would you need to have it spend next to the asteroid?

Love: About a year.

Fraser: But if it’s just about to do the flyby, you could give it a very small change and it would still kick it out of the bad orbit and into a good orbit.

Love: Right, you’re going to use that flyby of the Earth to multiply the tiny effect you put on the asteroid with your spacecraft before the flyby. And then after the flyby, the effect is much greater.

Fraser: So what’s the stage of your proposal now? What’s the future for it right now?

Love: Well it hard to know. Right now we’ve made a proposal, we’ve gotten the idea out there, and people are talking about it. My co-author, Ed Lu and I have written many scientific papers for publication, and none of them have received even a tenth as much attention as this one. So the idea’s out there, and we’ll see what happens. I think the debate will become much more pointed if we actually do discover an asteroid that’s on a collision path with the Earth. Then we’ll really need to get together and decide what we’re going to do about it.

Fraser: Well that’s my concern with the whole process of protecting the Earth from asteroids. There’s a lot of uncertainty in predicting when and where an asteroid is going to hit. The better you can mark the orbit, the better you can know if it’s going to be a risk. In many cases, if you’ve got these ones that are 30 years out, decision makers and lawmakers might say: well, let’s wait until we know better. And yet, the more you know better, the less chance you have of changing its orbit.

Love: Yes, that’s always true, and human nature plays into this a lot. Nobody’s every suffered an asteroid strike, so it’s hard to compare it to things that we have suffered, like tsunamis and hurricanes to take a couple of recent examples. The things that we know about and experience in a person’s lifetime are always easier to visualize and understand. And to get people to pay attention to something that seems kind of esoteric and science fictiony; is this real, or are people just making it up? I don’t know a good solution to that, but the fact that people are talking about the idea and thinking about it – and not just in the elevated circles of academia – all over the world, I think is a good sign. At least we’re thinking about the problem and how to solve it.

First Galileo Satellite is in Orbit

GIOVE-A deploys its solar arrays. Image credit: ESA . Click to enlarge
The first Galileo demonstrator is in orbit, marking the very first step to full operability of Europe’s new global navigation satellite system, under a partnership between ESA and the European Commission (EC).

Giove A, the first Galileo in-orbit validation element, was launched today from Baikonur, Kazakhstan, atop a Soyuz-Fregat vehicle operated by Starsem. Following a textbook lift-off at 05:19 UTC (06:19 CET), the Fregat upper stage performed a series of manoeuvres to reach a circular orbit at an altitude of 23 258 km, inclined at 56 degrees to the Equator, before safely deploying the satellite at 09:01:39 UTC (10:01:39 CET).

“Years of fruitful cooperation between ESA and the EC have now provided a new facility in space for improving the life of European citizens on Earth” said ESA Director General Jean Jacques Dordain congratulating ESA and industrial teams on the successful launch.

This 600 kg satellite, built by Surrey Satellite Technology Ltd (SSTL) of Guildford, in the UK, has a threefold mission. First, it will secure use of the frequencies allocated by the International Telecommunications Union (ITU) for the Galileo system. Second, it will demonstrate critical technologies for the navigation payload of future operational Galileo satellites. Third, it will characterise the radiation environment of the orbits planned for the Galileo constellation.

Formerly known as GSTB-V2/A (Galileo System Test Bed Version 2), Giove A carries two redundant, small-size rubidium atomic clocks, each with a stability of 10 nanoseconds per day, and two signal generation units, one able to generate a simple Galileo signal and the other, more representative Galileo signals. These two signals will be broadcast through an L-band phased-array antenna designed to cover all of the visible Earth under the satellite. Two instruments will monitor the types of radiation to which the satellite is exposed during its two year mission.

The satellite is under the control of SSTL’s own ground station. All systems are performing well, the solar arrays are deployed and in-orbit checkout of the satellite has begun. Once the payload is activated, the Galileo signals broadcast by Giove A will be carefully analysed by ground stations to make sure they satisfy the criteria of the ITU filings.

First step for Galileo

A second demonstrator satellite, Giove B, built by the European consortium Galileo Industries, is currently being tested and will be launched later. It is due to demonstrate the Passive Hydrogen Maser (PHM), which, with a stability better than 1 nanosecond per day, will be the most accurate atomic clock ever launched into orbit. Two PHMs will be used as primary clocks onboard the operational Galileo satellites, with two rubidium clocks serving as backups.

Subsequently, four operational satellites will be launched to validate the basic Galileo space and related ground segments. Once this In-Orbit Validation (IOV) phase is completed, the remaining satellites will be launched to achieve Full Operational Capability (FOC).

Galileo will be Europe’s own global navigation satellite system, providing a highly accurate, guaranteed global positioning service under civilian control. It will be inter-operable with the US Global Positioning System (GPS) and Russia’s Global Navigation Satellite System (Glonass), the two other global satellite navigation systems. Galileo will deliver real-time positioning accuracy down to the metric range with unrivaled integrity.

Numerous applications are planned for Galileo, including positioning and derived value-added services for transport by road, rail, air and sea, fisheries and agriculture, oil prospecting, civil protection activities, building, public works and telecommunications.

Original Source: ESA Portal

Chandra Looks at the Earth’s Aurora

Low-energy X-rays are generated during auroral activity. Image credit: NASA. Click to enlarge
A team of scientists observed Earth’s north polar region ten times during a four-month period in 2004. As the bright arcs in this sample of images show, they discovered low-energy (0.1 – 10 kilo electron volts) X-rays generated during auroral activity. Other satellite observatories had previously detected high-energy X-rays from Earth’s auroras.

The images – seen here superimposed on a simulated image of the Earth – are from approximately 20-minute scans during which Chandra was pointed at a fixed point in the sky while the Earth’s motion carried the auroral region through the field of view. The color code of the X-ray arcs represents the brightness of the X-rays, with maximum brightness shown in red.

Auroras are produced by solar storms that eject clouds of energetic charged particles. These particles are deflected when they encounter the Earth’s magnetic field, but in the process large electric voltages are created. Electrons trapped in the Earth’s magnetic field are accelerated by these voltages and spiral along the magnetic field into the polar regions. There they collide with atoms high in the atmosphere and emit X-rays.

Original Source: Chandra X-ray Observatory

Ithaca Chasma on Tethys

Tethys shows off its great scar. Image credit: NASA/JPL/SSI Click to enlarge
A crescent Tethys shows off its great scar, Ithaca Chasma, for which the moon is renowned. The chasm is 100 kilometers (60 miles) across on average, and is 4 kilometers (2 miles) deep in places.

See Steep Scarps for a much closer view of the chasm taken during a Cassini flyby.

Ithaca Chasma is the most prominent sign of ancient geologic activity on Tethys (1,071 kilometers, or 665 miles across), whose surface is characterized principally by heavy cratering.

The lit surface visible here is on the moon’s Saturn-facing hemisphere. North on Tethys is straight up.

The image was taken with the Cassini spacecraft narrow-angle camera on Nov. 28, 2005 using a filter sensitive to wavelengths of infrared light centered at 930 nanometers. The view was acquired at a distance of approximately 1.1 million kilometers (700,000 miles) from Tethys and at a Sun-Tethys-spacecraft, or phase, angle of 123 degrees. Resolution in the original image was 6 kilometers (4 miles) per pixel. The image has been magnified by a factor of two and contrast-enhanced to aid visibility.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org .

Original Source: NASA/JPL/SSI News Release