China's Main Competitor in Space Exploration is India, Not Russia

China's principal competitor in space exploration is India, not Russia, researcher at the Russian Centre for Analysis of Strategies and Technologies Vasily Kashin told RIA Novosti on Friday.

"China and India are two new space powers. They have vast resources and consider their space programs from the national prestige perspective ," the expert said.

He added that China and India are following Russian and US footsteps in space exploration.

"China's more developed space-rocket industry and immense resources have let it take the lead in the two countries' space race," Kashin argued.

Despite being behind China in space exploration, India has a significant advantage, according to the researcher.

"China is still under rigid restrictions on any form of cooperation with the United States, including on the purchase of components...The Chinese are forced to do many things on their own and they sometimes cannot produce components of a required level. The Indians have less resources, but they are in good relations with everyone. India can cooperate with both Russia and the West, adopting their best technologies," Kashin concluded.

Earlier on Friday, China launched an experimental spacecraft to the moon orbit, which is to return to Earth in eight days. The spacecraft is to test out re-entry into the Earth's atmosphere for the planned 2017 Chang'e-5 lunar mission.

Czech Republic prepares own space program

The Czech Republic will have its own space program, according to the National Space Plan for 2014-2019 that the government approved at the beginning of the week, the daily Hospodárske noviny (HN) writes today.
The plan recommends that the National Space Agency, "a considerably smaller variant of NASA," be established to integrate the currently fragmented competences in this field, HN says.
So far the Czech Republic has participated in the European Space Agency (ESA) programs, the second most significant player in space exploration after NASA, which they joined in 2008. Czechs annually give some 14 million euros to the ESA.
The national space exploration program should have an annual budget of three to five million euros and last for five years at least.
It should complement the research carried out within the ESA. Consequently, the National Space Agency could fund the projects that cannot be paid by the ESA, HN says.
Jan Kolář, head of the Czech Space Office NGO, welcomes the idea of the national space program.
"However, it should focus on the preparation of research and development activities in technical sciences," such as the development of materials and various types of detectors and the aerodynamics area, Kolář said.
HN writes that one of the rare successes that Czech science and industry has recently scored in this filed is a micro-accelerometer used in the SWARM satellites that were sent into space last November. The device, developed by 15 Czech firms, measures slight and slow accelerations that influence the satellite's movement, which removes possible distortions in the magnetic field measurements, HN notes.
However, the successful Czech micro-accelerometer was rather an exceptional case, Kolář told HN.
He said Czech participation in the ESA is limited by finances on the one hand, and by skills on the other hand. "In addition, our participation in each program is confronted with other European countries," he added.
Under the approved national space plan, the Czech Republic's contribution to the ESA's optional programs must be doubled at least, HN writes.
The transitory six-year period, in which the Czech Republic as a new ESA member could use a special incentive program, ends this year. Almost a half of the Czech obligatory payments to the agency went to it.
After the Czech Republic, Poland and Romania entered the ESA, while Estonia and Hungary plan to do so, and now they can use the advantages of newcomers, HN adds.
Source : prague post

Finnish researchers discover new type of black hole

Researchers at the University of Turku, in cooperation with international colleagues, have identified a new type of low-mass black hole. The type now discovered is a bright celestial object that emits x-rays.


NOTE : It is not possible to directly observe a black hole, but it is possible to detect events in its vicinity. An artist's concept of x-ray emissions from a black hole, published by NASA, August 2014

This new type of black hole has less mass than other known types and is associated with x-ray emitting quasars.

Up until now, it has been assumed that the collapse of a massive star generally forms a massive black hole or a small neutron star. The mass gap between neutron stars and stellar mass black holes is a question that has been a matter of inquiry for numerous research teams.

The object now discovered and designed SWIFT J1753.5-0127 has a mass somewhere between that of a conventionally-recognized black hole and a neutron star. Previously, observed neutron stars have been found to have less than two solar masses, while black holes have over five.

Observations related to this new type of low-mass black hole were published in a paper by a group of reseachers at the University of Turku, the Osservatorio Astronomico di Padova, the Max-Planck-Institut für Astronomie, and the INAF-IASF Milan branch, and published by the Monthly Notices of the Royal Astronomical Society.

Source : yle

Evidence Builds for Dark Matter Explosions at the Milky Way’s Core

This Fermi map of the Milky Way center shows an overabundance of gamma-rays (red indicates the greatest number) that cannot be explained by conventional sources.

So far, dark matter has evaded scientists’ best attempts to find it. Astronomers know the invisible stuff dominates our universe and tugs gravitationally on regular matter, but they do not know what it is made of. Since 2009, however, suspicious gamma--ray light radiating from the Milky Way’s core—where dark matter is thought to be especially dense—has intrigued researchers. Some wonder if the rays might have been emitted in explosions caused by colliding particles of dark matter. Now a new gamma-ray signal, in combination with those already detected, offers further evidence that this might be the case.

One possible explanation for dark matter is that it is made of theorized “weakly interacting massive particles,” or WIMPs. Every WIMP is thought to be both matter and antimatter, so when two of them meet they should annihilate on contact, as matter and antimatter do. These blasts would create gamma-ray light, which is what astronomers see in abundance at the center of our galaxy in data from the Fermi Gamma-Ray Space Telescope. The explosions could also create cosmic-ray particles—high-energy electrons and positrons (the antimatter counterparts of electrons)—which would then speed out from the heart of the Milky Way and sometimes collide with particles of starlight, giving them a boost of energy that would bump them up into the gamma-ray range. For the first time scientists have now detected light that matches predictions for this second process, called inverse Compton scattering, which should produce gamma rays that are more spread out over space and come in a different range of energies than those released directly by dark matter annihilation.

“It looks pretty clear from their work that an additional inverse Compton component of gamma rays is present,” says Dan Hooper, an astrophysicist at the Fermi National Accelerator Laboratory who was not involved in the study, but who originally pointed out that a dark matter signal might be present in the Fermi telescope data. “Such a component could come from the same dark matter that makes the primary gamma-ray signal we've been talking about all of these years.” University of California, Irvine scientists Anna Kwa and Kevork Abazajian presented the new study October 23 at the Fifth International Fermi Symposium in Nagoya, Japan and submitted their paper to Physical Review Letters.

None of the intriguing gamma-ray light is a smoking gun for dark matter. Other astrophysical processes, such as spinning stars called pulsars, can create both types of signal. “You can make models that replicate all this with astrophysics,” Abazajian says. “But the case for dark matter is the easiest, and there’s more and more evidence that keeps piling up.”

The official Fermi telescope team has long been cautious about drawing conclusions on dark matter from their data. But at last week’s symposium, the group presented its own analysis of the unexplained gamma-ray light and concluded that although multiple hypotheses fit the data, dark matter fits best. “That’s huge news because it’s the first time they’ve acknowledged that,” Abazajian says. Simona Murgia, an astrophysicist at the University of California, Irvine and a member of the Fermi collaboration’s galactic-center analysis team, presented the team’s findings. She says the complexity of the galactic center makes it difficult to know for sure how the excess of gamma rays arose and whether or not the light could come from mundane “background” sources. “It is a very interesting claim,” she says of Abazajian’s analysis. “However, detection of extended excesses in this region of the sky is complicated by our incomplete understanding of the background.”

The dark matter interpretation would look more likely if astronomers could find similar evidence of WIMP annihilation in other galaxies, such as the two dozen or so dwarf galaxies that orbit the Milky Way. “Extraordinary claims require extraordinary evidence, and I think a convincing claim of discovery would probably require a corresponding signal in another location—or by a non-astrophysical experiment—as well as the galactic center,” says Massachusetts Institute of Technology astrophysicist Tracy Slatyer, who has also studied the Fermi data from the Milky Way’s center.

Non-astrophysical experiments include the handful of so-called direct-detection experiments on Earth, which aim to catch WIMPs on the extremely rare occasions when they bump into atoms of normal matter. So far, however, none of these has found any evidence for dark matter. Instead they have steadily whittled away at the tally of possible types of WIMPs that could exist.

Other orbiting experiments, such as the Alpha Magnetic Spectrometer (AMS) on the International Space Station, which detects cosmic rays, have also failed to find convincing proof of dark matter. In fact, the AMS results seem to conflict with the most basic explanations linking dark matter to the Fermi observations. “Most people would agree that there is something rather unexpected happening at the galactic center, and it would be tremendously exciting if it turns out to be a dark matter annihilation signal,” says Christoph Weniger of the University of Amsterdam, another astrophysicist who has studied the Milky Way’s core. “But we have to confirm this interpretation by finding corroborating evidence in other independent observations first. Much more work needs to be done.”

Source : scientificamerican

JAXA shows off second-generation asteroid explorer 'Hayabusa 2'

Japan's space agency showed off a space probe to be launched next month that it hopes will answer questions about how life seeded Earth.

The Japan Aerospace Exploration Agency (JAXA) intends to land Hayabusa 2 on an asteroid orbiting between Earth and Mars. It is set to be launched by an H-2A rocket from the Tanegashima Space Center here on Nov. 30.

Its predecessor, launched in 2003, returned to Earth after a seven-year mission, during which it landed on an asteroid and collected sample material, an unprecedented achievement.

JAXA showed off the near complete body of its second-generation asteroid explorer to reporters on Oct. 27.

Hayabusa 2 will embark on a six-year journey to collect samples from an asteroid called 1999 JU3. Scientists expect the mission to shed light on the origins of the solar system and life on Earth.

The spherical asteroid is about 900 meters diameter and is thought to contain organic compounds and water, the key to life. It was first observed in 1999.

Hayabusa 2 arrived at Tanegashima island, south of Kagoshima, on Sept. 22. The capsule, impactor and other parts were then assembled.

A JAXA official said Hayabusa 2 will be attached to the rocket after fueling operations are complete and the exterior of the explorer has been inspected for flaws.

Hayabusa 2 is slated to reach the asteroid between June and July in 2018, and spend 18 months on the celestial body before returning to Earth between November and December in 2020.

The explorer will release the impactor to smash a crater and collect mineral samples that have not been exposed to and affected by the heat of the sun.

Russian Cargo Ship Lifts Off For Space Station

An unmanned Russian cargo ship successfully lifted off for the International Space Station (ISS) on October 29.

The Progress 57 craft was launched atop a Soyuz rocket at 8:09 a.m. Prague time from the Russian-leased Baikonur facility in Kazakhstan.

"Everything looks good on the Soyuz booster and the Progress resupply ship," an announcer on the U.S. space agency's NASA TV said.

The launch came nine hours after a privately operated rocket exploded seconds after liftoff in the United States, causing the loss of cargo ship that was also bound for the ISS.

The explosion of the Antares was the first such accident since NASA turned to private operators to deliver cargo to the station, breaking a Russian monopoly that followed the retirement of the U.S. space shuttle fleet in 2011.

The Progress is delivering nearly three metric tons of propellant, oxygen, water, and other supplies to the station.

EXPLOSION OF NASA'S UNMANNED ROCKET ANTARES

An unmanned Antares rocket exploded seconds after liftoff from a commercial launch pad in Virginia on Tuesday, marking the first accident since NASA turned to private operators to deliver cargo to the International Space Station, but officials said no one was hurt.

The 14-story rocket, built and launched by Orbital Sciences Corp, blasted off its seaside launch pad at the Wallops Flight Facility at 6:22 p.m. EDT carrying a Cygnus cargo ship for the space station. It exploded in a huge fireball moments later.

Orbital Sciences stock was down 12.74 percent after hours, or down $3.87 at $26.50.

The cause of the accident was not immediately known, said NASA mission commentator Dan Huot.

Huot said there were no reports of any personnel in the vicinity of the explosion. An Accomack County Sheriff's spokeswoman added, "As far as we know, all personnel are accounted for and everyone's OK."

Orbital Sciences said in a statement: "We've confirmed that all personnel have been accounted for. We have no injuries in the operation today."

NASA launch control said damage appeared to be limited to the launch facility and rocket. The Antares rocket has been launched successfully on four previous missions.

"This has been a lot of hard work to get to this point," Orbital Sciences Executive Vice President Frank Culbertson told the launch team just before liftoff.

http://www.youtube.com/watch?v=hSJ2kcDirEo

Launch had been delayed one day after a boat sailed into a restricted safety zone beneath the rocket's intended flight path.

Virginia-based Orbital Sciences is one of two companies hired by NASA to fly cargo to the station after the space shuttles were retired. Tuesday's planned flight was to be the third of eight under the company's $1.9 billion contract with NASA.

The second U.S. supply line to the station is run by privately owned Space Exploration Technologies, or SpaceX, which is preparing for its fourth flight under a separate $1.6 billion NASA contract.

Outfitted with a new, more powerful upper-stage engine, the Antares rocket launched on Tuesday carried a Cygnus spacecraft packed with 5,055 pounds (2,293 kg) of supplies, science experiments and equipment, a 15 percent increase over previous missions.

Cygnus was to loiter in orbit until Nov. 2, then fly itself to the station so astronauts can use a robotic crane to snare the capsule and attach it to a berthing port. The station, a $100 billion research laboratory owned and operated by 15 nations, flies about 260 miles (418 km) above Earth.

In addition to food, supplies and equipment, the Cygnus spacecraft was loaded with more than 1,600 pounds (725 kg) of science experiments, including an investigation to chemically analyze meteors as they burn up in Earth’s atmosphere.

The Cygnus also carried a prototype satellite owned by Redmond, Washington-based startup Planetary Resources Inc., which is developing technology to mine asteroids. The satellite, designated A3, was to be released into space by a commercially owned small spacecraft launcher aboard the station.

Source : Reuters

High-Altitude Methane Ice Cloud Discovered Floating Above Titan's Pole

NASA scientists have uncovered a starting new find on Saturn's moon, Titan. They've found an unexpected high-altitude methane ice cloud, similar to exotic clouds formed high above Earth's own poles. This cloud in the stratosphere over Titan’s north pole (left) is similar to Earth’s polar stratospheric clouds (right). NASA scientists found that Titan’s cloud contains methane ice, which was not previously thought to form in that part of the atmosphere. Cassini first spotted the cloud in 2006. (Photo : L. NASA/JPL/U. of Ariz./LPGNantes; R. NASA/GSFC/M. Schoeberl)

NASA scientists have uncovered a starting new find on Saturn's moon, Titan. They've found an unexpected high-altitude methane ice cloud, similar to exotic clouds formed high above Earth's own poles.

The researchers first spotted the cloud with the help of NASA's Cassini spacecraft. It was part of the winter cap of condensation over Titan's north pole. Now, scientists have teased apart the data and found that the cloud contained methane ice, which produces a much denser cloud than the previously identified ethane ice.

"The idea that methane clouds could form this high on Titan is completely new," said Carrie Anderson, lead author of the new study, in a news release. "Nobody considered that possible before."

The temperatures in Titan's lower stratosphere are not the same at all latitudes. In fact, the high-altitude temperature near the north pole is far colder than just south of the equator. This temperature difference-as much as 11 degrees Fahrenheit-is enough to yield methane ice.

So how do these clouds form? The mechanisms for forming these high-altitude clouds are different from what happens in the troposphere. Titan has a global circulation pattern; warm air in the summer hemisphere wells up from the surface and enters the stratosphere, slowly making its way to the winter pole. There, the air sinks back down and cools as it descends. This forms the methane clouds.

Currently, the scientists are gathering more information about Saturn's moon in order to better understand the natural processes that occur on the alien world. This could shed light on the processes that occur on exoplanets and allow scientists to apply their findings to processes that also occur on Earth.

"Titan continues to amaze with natural processes similar to those on Earth, yet involving materials different from our familiar water," said Scott Edgington, Cassini deputy project scientist. "As we approach southern winter solstice on Titan, we will further explore how these cloud formation processes might vary with season."

Amazing picture of Supernova 1987A

Real image SN 1987A located at 1,68,000 light years from earth in Large Magellanic Cloud (Another Galaxy)

you can imagine the power of this supernova by understanding that even it was located at another galaxy it was visible to the naked eye. It was the first supernova that modern astronomers had to observe a SN and to use modern technology in that observation allowing them to gather much more data.

Supernovae are extremwely rare events. About 1 every 200 years is visible and they only last for a month or two.



image of SN 1987A

Popular Physicist Says , "We are alone in the universe"

The process which led to the creation of humankind on earth was a fluke - and it is highly unlikely it has been repeated anywhere else in the universe.

That is the view of English physicist Professor Brian Cox, who made the assertion in an episode of BBC's Human Universe.

Professor Cox thwarted suggestions alien life was a possibility and said he believed humans were the only form of life in the universe, despite the astronomical number of other planets in the galaxy.

The presenter and scientist, who also appeared on the ABC's Q&A program last week, blamed a series of "evolutionary bottlenecks" as the main reason no extraterrestrial life has been discovered.

"There is only one advanced technological civilisation in this galaxy and there has only ever been one - and that's us," Professor Cox said. "We are unique.

"It's a dizzying thought. There are billions of planets out there, surely there must have been a second genesis?
"But we must be careful because the story of life on this planet shows that the transition from single-celled life to complex life may not have been inevitable."

Professor Cox went on to say that the extinction of dinosaurs, believed by scientists to have been caused by a meteor impact, allowed mammals and ultimately humans to dominate the planet.

"We still struggle to understand how this happened," he said. "It's incredibly unusual.

"We're confident this only happened once in the oceans of the primordial earth. Life here did squeeze through."

Professor Cox's views are in stark contrast to those of astrophysicists Dr Timothy Brandt and Dr David Spiege of Princeton University, who last month made the claim that our best chance of finding aliens, if they exist at all, lies in the examination of plant life on planets outside our solar system, known as exoplanets.

They said if alien life existed on exoplanets, it might be possible to detect traces of water, oxygen and chlorophyll.

Meanwhile, NASA has offered a more widely accepted prediction; that one hundred million worlds in our galaxy are capable and fit to host alien life.

Spacecraft Spots Ice at Mercury's North Pole

NASA 's MESSENGER spacecraft has sent back its first visible-light images of water ice on Mercury, the tiny charbroiled planet that orbits closest to the sun.

The findings, described in the journal Geology, reveal that the ice deposits look surprisingly "fresh" -- and hint that water could have been very recently delivered to rocky little Mercury.

Even though Mercury sits less than 36 million miles from the sun -- which is less than two-fifths of the Earth's comfortable 93 million miles from sun -- some ice still manages to cling to the planet's surface. That's because the ice lies at the poles, in permanently shadowed regions inside craters that are eternally shielded from sunlight and remain very, very cold.

More than two decades ago, ground-based radar observations picked up signs of this polar ice, and the MESSENGER spacecraft later lent support to the idea with its own suite of instruments. But it's tough to actually see these permanently shadowed regions with the spacecraft's visible-light camera because, well, it's dark there. But recently, the team was able to refine the images of the ice-deposit surfaces with the help of what little light was reflecting off the crater walls.

The scientists examined Prokofiev, which at roughly 69.6 miles in diameter is the largest crater at Mercury's north pole thought to have water-ice deposits. There, the surface ice had a "cratered" texture -- showing that it was placed there more recently than the smaller underlying craters.

And in other spots, such as Berlioz crater, the researchers found that the water ice was "covered by a thin layer of dark, organic-rich volatile material." The boundaries of those icy regions were surprisingly sharp -- they hadn't been in place long enough to get smoothed out.

"The sharp boundaries indicate that the volatile deposits at Mercury's poles are geologically young, relative to the time scale for lateral mixing by impacts," the study authors wrote, "and either are restored at the surface through an ongoing process or were delivered to the planet recently."

To put that idea in perspective, estimates indicate that there could be roughly enough water-ice on Mercury to fill Lake Ontario. And if at least some of that water is indeed being delivered to the planet, it sheds new light on dynamics in the inner solar system, the scientists said.

"If Mercury's currently substantial polar volatile inventory is the product of the most recent portion of a longer process," the study authors wrote, "then a considerable mass of volatiles may have been delivered to the inner Solar System throughout its history."