Posts Tagged space.com

Space Junk

The already untidy mass of orbital debris that litters low Earth orbit nearly got nastier last month. A head-on collision was averted between a spent upper stage from a Chinese rocket and the European Space Agency’s (ESA) huge Envisat Earth remote-sensing spacecraft.Space junk tracking information supplied by the U.S. military, as well as confirming German radar data, showed that the two space objects would speed by each other at a nail-biting distance of roughly 160 feet (50 meters).

ESA’s Envisat tips the scales at 8 tons, with China’s discarded rocket body weighing some 3.8 tons. A couple of tweaks of maneuvering propellant were used to nudge the large ESA spacecraft to a more comfortable miss distance. But what if the two objects had tangled?

Such a space collision would have caused mayhem in the heavens, adding clutter to an orbit altitude where there are big problems already, said Heiner Klinkrad, head of the European Space Agency’s Space Debris Office in Darmstadt, Germany.

It turns out, Klinkrad told SPACE.com, that 50 percent of all the close conjunctions that Envisat faces are due to the lethal leftovers from China’s January 2007 anti-satellite test, as well as chunks of junk resulting from last year’s smashup between an active U.S. Iridium satellite and a defunct Russian Cosmos spacecraft.

Klinkrad joined several orbital debris experts that took part in the 33rd Annual Guidance and Control Conference organized by the Rocky Mountain Section of the American Astronautical Society. The five-day meeting began Feb. 5.

Avoidance maneuvers

Significant progress has been made by the U.S. and the international aerospace communities in recognizing the hazards of orbital debris, reported Nicholas Johnson, chief scientist for orbital debris at the NASA Johnson Space Center in Houston, Texas.

Johnson added that steps are being taken to reduce or eliminate the potential for the creation of new debris. However, “the future environment is expected to worsen without additional corrective measures,” he noted.
During 2009, Johnson reported, five different NASA robotic spacecraft carried out collision avoidance maneuvers: a Tracking and Data Relay Satellite (TDRS-3), Cloudsat, Earth Observing Mission 1, Aqua, and Landsat 7. Also, the space shuttle and the International Space Station took collision avoidance actions, he said.

The worst thing that could happen, according to ESA’s Klinkrad, is the International Space Station (ISS) receiving a fatal hit. The space station is currently home to five astronauts representing the U.S., Russia and Japan. “A penetrating object hitting the ISS, and possibly causing a casualty onboard . . . I think that would be the most dramatic case we could have,” Klinkrad suggested. Such an incident might turn public opinion against human spaceflight, he said.

Collaboration on the increase

One bit of good news in all this orbital riff-raff. Due to last year’s satellite crash between the Iridium and Cosmos spacecraft, Johnson explained that the Joint Space Operations Center (JSpOC) of the U.S. Strategic Command now conducts conjunction assessments for all operational spacecraft in Earth orbit, regardless of ownership nationality. “To be honest, a year ago, we couldn’t even have hoped to have done this,” Johnson told SPACE.com.

“It’s really a consequence of the collision last year. People have been talking about this for years. But now we’ve made the commitment . . . that this is something that needs to be done and can be done relatively easily,” Johnson said. Klinkrad concurred. “The collaboration is getting even closer now,” he said.

Duck or pluck?

Playing dodge ball with high-speed space debris is one tactic. But there is also a growing interest in removing the most troublesome objects — perhaps an annual quota of some sort.Targeted would be specific inclination bands and altitude regimes, Klinkrad said. But prior to implementing debris remediation measures on a global scale, technical, operational, legal and economic problems must be overcome. Klinkrad and NASA’s Johnson provided a wearisome appraisal of the future.

Even with an immediate halt of launch activities, spacefaring nations will be dealing with an unstable low-Earth orbit environment in some altitude and inclination bands. This would be a consequence of about 20 catastrophic collisions within the next 200 years, the two orbital debris experts explained. Some orbit altitudes already have critical mass concentrations that will trigger “collisional cascading” within a few decades, unless debris environment remediation measures are introduced.

The Kessler Syndrome

The idea of debris creating debris was put in motion by Donald Kessler, along with fellow NASA researcher, Burton Cour-Palais, back in 1978. Their research suggested that, as the number of artificial satellites in Earth orbit increases, the probability of collisions between satellites also increases. Satellite collisions would produce orbiting fragments, each of which would increase the probability of further collisions, leading to the growth of a belt of debris around the Earth.Now, decades later, that prophecy has been dubbed the Kessler Syndrome.

Kessler told SPACE.com that the disorder fits into much more complex natural laws that include the evolution of the solar system, as well as meteoroids, meteorites, and climate-changing asteroids. Kessler is now an orbital debris and meteoroid consultant in Asheville, North Carolina.”There is nothing complex about what is called the ‘Kessler Syndrome’ . . . it is just the way nature may have converted a disorderly group of orbiting rocks into an orderly solar system . . . although nature reminds us with a large asteroid or comet collision every few million years that it isn’t quite finished yet. “In the case of orbital debris, this collision process is just starting,” Kessler explained. Consequently, nobody should be surprised that as orbital debris models became more complex — and as more data is obtained — the same conclusion holds, Kessler said.

“The future debris environment will be dominated by fragments resulting from random collisions between objects in orbit, and that environment will continue to increase, even if we do not launch any new objects into orbit,” Kessler concluded.


http://www.space.com/missionlaunches…er-100223.html

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Water Planet Discovered

A rocky and water-rich planet, not much heftier than our own, has been discovered so close to our solar system that astronomers one day may be able to study its atmosphere. And though astronomers are pretty certain the water exists, they don’t know its state, with speculations ranging from liquid water to water ice and an exotic state called a superfluid. The extrasolar planet, now named GJ 1214b, is about 40 light-years away. It orbits a red dwarf star. It is the only known “Super-Earth” exoplanet — worlds that have masses between Earth and Neptune — with a confirmed atmosphere. “Astronomically speaking, this [planet] is on our block,” meaning it’s in our cosmic neighborhood, said study leader David Charbonneau of the Harvard-Smithsonian Center for Astrophysics in Mass. “For perspective, our own TV signals have already passed beyond the distance of this star.” The planet is about three times the size of Earth and about 6.5 times as massive. It is the second smallest planet discovered outside of our solar system to date, trailing behind only CoRoT-7b, which is 1.7 times Earth’s size and about five times as massive.

GJ 1214b is rare among known rocky exoplanets because it partially eclipses, or transits, its star as seen from Earth. This fortunate alignment allows astronomers to calculate the size and density of the planet, and Charbonneau’s team thinks GJ 1214b is likely a water world with a solid center. Moreover, the planet has a thick surrounding atmosphere of hydrogen and helium.

Normally, a planet located at that distance from this particular type of star would be so hot that any water on its surface would be in a vapor form. But scientists think the thick atmosphere of GJ 1214b creates a high pressure environment that keeps water on the surface in a liquid state. That’s just speculation, however.

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Massive Supernova

Supernova

Supernova

All supernova explosions are violent affairs, but this one takes the cake. Astronomers have spotted a new type of extremely bright cosmic explosion they think originates from an exceptionally massive star. This breed of explosion has been long predicted, but never before seen. Like all supernovas, the blast is thought to have marked the end of a star’s life. But in this case, that star may have started out with 200 times the mass of the sun. The supernova in question, SN2007bi, was observed in 2007 in a nearby dwarf galaxy. Scientists knew at once it was something different because it was about 50 to 100 times brighter than a typical supernova.

“It was much brighter, and it was bright for a very long time,” said researcher Paolo Mazzali of the Max-Planck Institute for Astrophysics in Germany. “We could observe this thing almost two years after it was discovered, where you normally don’t see anything anymore.” After analyzing its signature, astronomers published a paper in the Dec. 3 issue of the journal Nature confirming that it matches theoretical predictions of a so-called pair-instability supernova. “There were some doubts that they existed,” said astronomer Norbert Langer of the University of Bonn in Germany, who did not work on the project. Langer wrote an opinion essay on the finding in the same issue of Nature. “There were severe doubts that stars that massive could ever form in the universe. Now we seem to be very sure that there was a star with 200 solar masses.”

In a pair-instability supernova, the star has neared the end of its life and exhausted its main supplies of hydrogen and helium, leaving it a core of mostly oxygen. In smaller stars, the core continues to burn until eventually it is all iron, then collapses in a Type II supernova, leaving behind a remnant black hole or neutron star. But in the case of an extremely massive star, while its core is still made of oxygen, it releases photons that are so energetic, they create pairs of electrons and their anti-matter opposites, positrons. When the matter and antimatter meet, they annihilate each other. This reaction reduces the star’s pressure, and it collapses, igniting the oxygen core in a runaway nuclear explosion that eats up the whole star, leaving no remnant at all.

The discovery of this rare type of supernova suggests that a few stars actually can grow into such large behemoths — which has long been a topic of debate. “I was never a believer in very massive stars,” Mazzali told SPACE.com. “Seeing something like this explode means these things exist. This is a fairly new development in the formation of stars.”

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