New Studies Propose Two New Planets Beyond Pluto

New calculations from an international team of researchers suggest that there could be two unknown planets beyond Pluto.

In two new studies, published in the Monthly Notices of the Royal Astronomical Society, scientists from the University of Madrid and the University of Cambridge posit that two, or more, unknown planets are responsible for unusual behaviour beyond Neptune.

Objects, in that far-flung part of the Solar System, don’t act like we believe they should: the paths they move along do not have the orbital inclinations and axes that astronomers would expect to see, based on current theory of what researchers call "trans-Neptunian objects."

Unless, the astrophysicists posit, there’s something else out there, and, after considering the effects of the “Kozai mechanism,” the effect an object orbiting further out from a gravitational source can have one orbiting futher in, they now believe there are at least two mysterious planets at play.

“Our results may be truly revolutionary for astronomy,” says co-author Carlos de la Fuente Marcos in a news release, but the team says this is still a hypothesis.

To prove it, scientists will have to overcome two hurdles. Not only does the new theory challenge astrophysicists' current thinking about how the solar system came to be, but the sample size used in the study’s calculations contains only 13 objects.

However, the team promises that with a larger sample size, coming soon, and new research (a recently-discovered planet-in-process is much further away from a star than scientists suspected to be possible), they’ll soon have even more evidence that our solar system may be even bigger than thought.

More Information
'Flipping minor bodies: what comet 96P/Machholz 1 can tell us about the orbital evolution of extreme trans-Neptunian objects and the production of near-Earth objects on retrograde orbits' published in the Monthly Notices of the Royal Astronomical Society - 10.1093/mnras/stu2230

Hubble Begins Search Beyond Pluto For Potential Flyby Targets

This is an artist's rendering of the New Horizons spacecraft encountering a Kuiper Belt object - a city-sized icy relic left over from the birth of our solar system. 

The sun, more than 4.1 billion miles (6.7 billion kilometers) away, shines as a bright star embedded in the glow of the zodiacal dust cloud. 

Jupiter and Neptune are visible as orange and blue "stars" to the right of the sun. 

Image courtesy JHUAPL /SwRI.

After careful consideration and analysis, the Hubble Space Telescope Time Allocation Committee has recommended using Hubble to search for an object the Pluto-bound NASA New Horizons mission could visit after its flyby of Pluto in July 2015.

The planned search will involve targeting a small area of sky in search of a Kuiper Belt object (KBO) for the outbound spacecraft to visit.

The Kuiper Belt is a vast debris field of icy bodies left over from the solar system's formation 4.6 billion years ago.

A KBO has never been seen up close because the belt is so far from the sun, stretching out to a distance of 5 billion miles into a never-before-visited frontier of the solar system.

"I am pleased that our science peer-review process arrived at a consensus as to how to effectively use Hubble's unique capabilities to support the science goals of the New Horizons mission," said Matt Mountain, director of the Space Telescope Science Institute (STScI) in Baltimore, Maryland.

Fully carrying out the KBO search is contingent on the results from a pilot observation using Hubble data.

The space telescope will scan an area of sky in the direction of the constellation Sagittarius to try and identify any objects orbiting within the Kuiper Belt.

To discriminate between a foreground KBO and the clutter of background stars in Sagittarius, the telescope will turn at the predicted rate that KBOs are moving against the background stars.

In the resulting images, the stars will be streaked, but any KBOs should appear as pinpoint objects.

If the test observation identifies at least two KBOs of a specified brightness it will demonstrate statistically that Hubble has a chance of finding an appropriate KBO for New Horizons to visit.

At that point, an additional allotment of observing time will continue the search across a field of view roughly the angular size of the full moon.

Astronomers around the world apply for observing time on the Hubble Space Telescope. Competition for time on the telescope is extremely intense and the requested observing time significantly exceeds the observing time available in a given year.

Proposals must address significant astronomical questions that can only be addressed with Hubble's unique capabilities, and are beyond the capabilities of ground-based telescopes.

The proposals are peer reviewed annually by an expert committee, which looks for the best possible science that can be conducted by Hubble and recommends to the Space Telescope Science Institute director a balanced program of small, medium, and large investigations.

Though Hubble is powerful enough to see galaxies near the horizon of the universe, finding a KBO is a challenging needle-in-haystack search.

A typical KBO along the New Horizons trajectory may be no larger than Manhattan Island and as black as charcoal.

NASA Cassini Image: Looking beyond Saturn to view Uranus

This view from NASA's Cassini spacecraft features a blue planet, but unlike the view from July 19, 2013 (PIA17172 The Day the Earth Smiled) that featured our home planet, this blue orb is Uranus, imaged by Cassini for the first time.

Credit: NASA /JPL-Caltech /Space Science Institute

Uranus is a pale blue in this natural colour image because its visible atmosphere contains methane gas and few aerosols or clouds.

Methane on Uranus and its sapphire-coloured sibling, Neptune, absorbs red wavelengths of incoming sunlight, but allows blue wavelengths to escape back into space, resulting in the predominantly bluish color seen here.

Cassini imaging scientists combined red, green and blue spectral filter images to create a final image that represents what human eyes might see from the vantage point of the spacecraft.

Uranus

Uranus has been brightened by a factor of 4.5 to make it more easily visible. The outer portion of Saturn's A ring, seen at bottom right, has been brightened by a factor of two.

The bright ring cutting across the image center is Saturn's narrow F ring.

Uranus was approximately 28.6 astronomical units from Cassini and Saturn when this view was obtained.

An astronomical unit is the average distance from Earth to the sun, equal to 93,000,000 miles (150,000,000 kilometers).

Neptune

The view was acquired by the Cassini narrow-angle camera at a distance of approximately 614,300 miles (988,600 kilometers) from Saturn on April 11, 2014.

Image scale at Uranus is approximately 16,000 miles (25,700 kilometers) per pixel.

Image scale at Saturn's rings is approximately 4 miles (6 kilometers) per pixel.

In the image, the disk of Uranus is just barely resolved.

The solar phase angle at Uranus, seen from Cassini, is 11.9 degrees.

Russian Cosmonaut Alexander Misurkin: Humankind should explore the Solar System and beyond

Alexander Misurkin

Alexander Misurkin. Image courtesy RIA Novosti and Ramil Sitdikov.

Russian astronaut Alexander Misurkin thinks humankind should not stop at the exploration of near-Earth space but rather go further in the universe, the explorer told RIA Novosti Tuesday.

"I think, we shouldn't limit ourselves to exploring the Earth's orbit. I, personally, would be interested in going to the outer space, exploring the asteroids, the Moon, and Mars. It's a natural development for me, we have no right to stop at the orbit of our planet," Misurkin said.

Misurkin was part of the international space station crew coming back to Earth in September 2013.

The astronauts carried out 45 scientific research tasks in the 166 days they spent on board of the station.

Fyodor Yurchikhin

Alexander Misurkin and Fyodor Yurchikhin went into open space working there for 7,5 hours hitting record time for a Russian-made spacesuit.

"Coming back to the orbit is a logical development, because astronaut training is extremely expensive for just one flight," he said expressing his willingness to participate in another space expedition.

Misurkin thinks that US sanctions on Russia can deal a heavy blow to space cooperation.

"I am more than sure that great achievements in space require collaborative work, there is no alternative here. I really hope this doesn't happen and we continue cooperation all the while involving more and more countries in it," the astronaut said.

Robotic Refueling: The Jumpstart Push Beyond LEO

On July 12, 2011, spacewalking astronauts Mike Fossum and Ron Garan successfully transferred the Robotic Refueling Mission, or RRM, module from the Atlantis shuttle cargo bay to a temporary platform on the International Space Station's Dextre robot.

Credit: NASA

In mid-January, NASA will take the next step in advancing robotic satellite-servicing technologies as it tests the Robotic Refueling Mission (RRM) aboard the International Space Station.

The investigation may one day substantially impact the many satellites that deliver products Americans rely upon daily, such as weather reports, cell phones and television news.

During five days of operations, controllers from NASA and the Canadian Space Agency will use the space station's remotely operated Special Purpose Dexterous Manipulator (Dextre), robot to simulate robotic refueling in space.

Operating a space-based robotic arm from the ground is a feat on its own, but NASA will do more than just robotics work as controllers remotely snip wires, unscrew caps and transfer simulated fuel.

The team also will demonstrate tools, technologies and techniques that could one day make satellites in space greener, more robust and more capable of delivering essential services to people on Earth.

Fix or Refuel a Satellite?

"Every satellite has a lifespan and eventual retirement date, determined by the reliability of its components and how much fuel it can carry," explains Benjamin Reed, deputy project manager of NASA's Satellite Servicing Capabilities Office (SSCO).

Repairing and refueling satellites already in place, Reed asserts, can be far less expensive than building and launching entirely new spacecraft, potentially saving millions, even billions of dollars and many years of work.

The RRM demonstration specifically tests what it would take to repair and refuel satellites traveling the busy space highway of geosynchronous Earth orbit, or GEO.

Located about 22,000 miles above Earth, this orbital path is home to more than 400 satellites, many of which beam communications, television and weather data to customers worldwide.

By developing robotic capabilities to repair and refuel GEO satellites, NASA hopes to add precious years of functional life to satellites and expand options for operators who face unexpected emergencies, tougher economic demands and aging fleets.

NASA also hopes that these new technologies will help boost the commercial satellite-servicing industry that is rapidly gaining momentum.

JWST: "Infrared: Beyond the Visible" explores the wonder of infrared astronomy

The answers to some of the universe's greatest cosmic mysteries are written across the night sky, inscribed in light we can't see with our human eyes — but it won't be invisible to us forever.

"Infrared: Beyond the Visible" explores the wonder of infrared astronomy and the promise of the upcoming Webb Space Telescope.

Get a sense of the sights Webb will capture, with its Hubble-sharp vision and ability to reach into the farthest depths of space and time.

Join the journey of discovery, and when you're done, check out the other links for more on the infrared universe.

Who wants to live forever? Who dares.......?