Saturday, June 29, 2013

ScienceDaily: Astronomy News

ScienceDaily: Astronomy News


NASA launches satellite to study how sun's atmosphere is energized

Posted: 28 Jun 2013 11:48 AM PDT

NASA's Interface Region Imaging Spectrograph (IRIS) spacecraft launched Thursday at 7:27 p.m. PDT (10:27 p.m. EDT) from Vandenberg Air Force Base, Calif. The mission to study the solar atmosphere was placed in orbit by an Orbital Sciences Corporation Pegasus XL rocket.

Friday, June 28, 2013

NASA Decommissions Its Galaxy Hunter Spacecraft

JPL/NASA News

News release: 2013-211                                                                    June 28, 2013

NASA Decommissions Its Galaxy Hunter Spacecraft

This image from NASA's Galaxy Evolution Explorer (GALEX) shows Messier 94, also known as NGC 4736, in ultraviolet light

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-211&cid=release_2013-211

PASADENA, Calif. -- NASA has turned off its Galaxy Evolution Explorer (GALEX) after a decade of operations in which the venerable space telescope used its ultraviolet vision to study hundreds of millions of galaxies across 10 billion years of cosmic time.

"GALEX is a remarkable accomplishment," said Jeff Hayes, NASA's GALEX program executive in Washington. "This small Explorer mission has mapped and studied galaxies in the ultraviolet, light we cannot see with our own eyes, across most of the sky."

Operators at Orbital Sciences Corporation in Dulles, Va., sent the signal to decommission GALEX at 12:09 p.m. PDT (3:09 p.m. EDT) Friday, June 28. The spacecraft will remain in orbit for at least 65 years, then fall to Earth and burn up upon re-entering the atmosphere. GALEX met its prime objectives and the mission was extended three times before being cancelled.


Highlights from the mission's decade of sky scans include:

-- Discovering a gargantuan, comet-like tail behind a speeding star called Mira.
-- Catching a black hole "red-handed" as it munched on a star.
-- Finding giant rings of new stars around old, dead galaxies.
-- Independently confirming the nature of dark energy.
-- Discovering a missing link in galaxy evolution -- the teenage galaxies transitioning from young to old.

The mission also captured a dazzling collection of snapshots, showing everything from ghostly nebulas to a spiral galaxy with huge, spidery arms.

In a first-of-a-kind move for NASA, the agency in May 2012 loaned GALEX to the California Institute of Technology in Pasadena, which used private funds to continue operating the satellite while NASA retained ownership. Since then, investigators from around the world have used GALEX to study everything from stars in our own Milky Way galaxy to hundreds of thousands of galaxies 5 billion light-years away.

In the space telescope's last year, it scanned across large patches of sky, including the bustling, bright center of our Milky Way. The telescope spent time staring at certain areas of the sky, finding exploded stars, called supernovae, and monitoring how objects, such as the centers of active galaxies, change over time. GALEX also scanned the sky for massive, feeding black holes and shock waves from early supernova explosions.

"In the last few years, GALEX studied objects we never thought we'd be able to observe, from the Magellanic Clouds to bright nebulae and supernova remnants in the galactic plane," said David Schiminovich of Columbia University, N.Y., N.Y, a longtime GALEX team member who led science operations over the past year. "Some of its most beautiful and scientifically compelling images are part of this last observation cycle."

Data from the last year of the mission will be made public in the coming year.

"GALEX, the mission, may be over, but its science discoveries will keep on going," said Kerry Erickson, the mission's project manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

A slideshow showing some of the popular GALEX images is online at: http://go.nasa.gov/17xAVDd

JPL managed the GALEX mission and built the science instrument. The mission's principal investigator, Chris Martin, is at Caltech. NASA's Goddard Space Flight Center in Greenbelt, Md., developed the mission under the Explorers Program it manages. Researchers sponsored by Yonsei University in South Korea and the Centre National d'Etudes Spatiales (CNES) in France collaborated on the mission. Caltech manages JPL for NASA.

Graphics and additional information about the Galaxy Evolution Explorer are online at: http://www.nasa.gov/galex

Media contact:

Alan Buis 818-354-0474
Jet Propulsion Laboratory, Pasadena, Calif.
alan.d.buis@jpl.nasa.gov

J.D. Harrington 202-358-5241
Headquarters, Washington
j.d.harrington@nasa.gov

2013-211


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ScienceDaily: Stars News

ScienceDaily: Stars News


Violent birth of neutron stars: Computer simulations confirm sloshing and spiral motions as stellar matter falls inward

Posted: 27 Jun 2013 05:30 AM PDT

Scientists have conducted the most expensive and most elaborate computer simulations so far to study the formation of neutron stars at the center of collapsing stars with unprecedented accuracy. These worldwide first three-dimensional models with a detailed treatment of all important physical effects confirm that extremely violent, hugely asymmetric sloshing and spiral motions occur when the stellar matter falls towards the center. The results of the simulations thus lend support to basic perceptions of the dynamical processes that are involved when a star explodes as supernova.

ScienceDaily: Galaxies News

ScienceDaily: Galaxies News


Spiral galaxies like Milky Way bigger than thought

Posted: 27 Jun 2013 07:26 AM PDT

Let's all fist bump: Spiral galaxies like our own Milky Way appear to be much larger and more massive than previously believed, according to a new study.

ScienceDaily: Cosmic Rays News

ScienceDaily: Cosmic Rays News


NASA's Voyager 1 explores final frontier of our 'solar bubble'

Posted: 27 Jun 2013 11:08 AM PDT

Data from Voyager 1, now more than 11 billion miles (18 billion kilometers) from the sun, suggest the spacecraft is closer to becoming the first human-made object to reach interstellar space.

ScienceDaily: Astronomy News

ScienceDaily: Astronomy News


Gas-giant exoplanets cling close to their parent stars

Posted: 27 Jun 2013 01:14 PM PDT

Gemini Observatory's Planet-Finding Campaign finds that, around many types of stars, distant gas-giant planets are rare and prefer to cling close to their parent stars. The impact on theories of planetary formation could be significant.

NASA's Voyager 1 explores final frontier of our 'solar bubble'

Posted: 27 Jun 2013 11:08 AM PDT

Data from Voyager 1, now more than 11 billion miles (18 billion kilometers) from the sun, suggest the spacecraft is closer to becoming the first human-made object to reach interstellar space.

Spiral galaxies like Milky Way bigger than thought

Posted: 27 Jun 2013 07:26 AM PDT

Let's all fist bump: Spiral galaxies like our own Milky Way appear to be much larger and more massive than previously believed, according to a new study.

Sterilizing Mars spacecraft is largely a waste of money, two experts argue

Posted: 27 Jun 2013 07:26 AM PDT

Two university researchers say environmental restrictions have become unnecessarily restrictive and expensive -- on Mars.

Violent birth of neutron stars: Computer simulations confirm sloshing and spiral motions as stellar matter falls inward

Posted: 27 Jun 2013 05:30 AM PDT

Scientists have conducted the most expensive and most elaborate computer simulations so far to study the formation of neutron stars at the center of collapsing stars with unprecedented accuracy. These worldwide first three-dimensional models with a detailed treatment of all important physical effects confirm that extremely violent, hugely asymmetric sloshing and spiral motions occur when the stellar matter falls towards the center. The results of the simulations thus lend support to basic perceptions of the dynamical processes that are involved when a star explodes as supernova.

ScienceDaily: Extrasolar Planets News

ScienceDaily: Extrasolar Planets News


Gas-giant exoplanets cling close to their parent stars

Posted: 27 Jun 2013 01:14 PM PDT

Gemini Observatory's Planet-Finding Campaign finds that, around many types of stars, distant gas-giant planets are rare and prefer to cling close to their parent stars. The impact on theories of planetary formation could be significant.

Thursday, June 27, 2013

NASA's Voyager 1 Explores Final Frontier of Our 'Solar Bubble'

JPL/NASA News
News release: 2013-209                                                             June 27, 2013

NASA's Voyager 1 Explores Final Frontier of Our 'Solar Bubble'

This artist's concept shows NASA's two Voyager spacecraft exploring a turbulent region of space known as the heliosheath, the outer shell of the bubble of charged particles around our sun

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-209&cid=release_2013-209

PASADENA, Calif. -- Data from Voyager 1, now more than 11 billion miles (18 billion kilometers) from the sun, suggest the spacecraft is closer to becoming the first human-made object to reach interstellar space.

Research using Voyager 1 data and published in the journal Science today provides new detail on the last region the spacecraft will cross before it leaves the heliosphere, or the bubble around our sun, and enters interstellar space. Three papers describe how Voyager 1's entry into a region called the magnetic highway resulted in simultaneous observations of the highest rate so far of charged particles from outside heliosphere and the disappearance of charged particles from inside the heliosphere.

Scientists have seen two of the three signs of interstellar arrival they expected to see: charged particles disappearing as they zoom out along the solar magnetic field, and cosmic rays from far outside zooming in. Scientists have not yet seen the third sign, an abrupt change in the direction of the magnetic field, which would indicate the presence of the interstellar magnetic field.

"This strange, last region before interstellar space is coming into focus, thanks to Voyager 1, humankind's most distant scout," said Ed Stone, Voyager project scientist at the California Institute of Technology in Pasadena. "If you looked at the cosmic ray and energetic particle data in isolation, you might think Voyager had reached interstellar space, but the team feels Voyager 1 has not yet gotten there because we are still within the domain of the sun's magnetic field."

Scientists do not know exactly how far Voyager 1 has to go to reach interstellar space. They estimate it could take several more months, or even years, to get there. The heliosphere extends at least 8 billion miles (13 billion kilometers) beyond all the planets in our solar system. It is dominated by the sun's magnetic field and an ionized wind expanding outward from the sun. Outside the heliosphere, interstellar space is filled with matter from other stars and the magnetic field present in the nearby region of the Milky Way.

Voyager 1 and its twin spacecraft, Voyager 2, were launched in 1977. They toured Jupiter, Saturn, Uranus and Neptune before embarking on their interstellar mission in 1990. They now aim to leave the heliosphere. Measuring the size of the heliosphere is part of the Voyagers' mission.

The Science papers focus on observations made from May to September 2012 by Voyager 1's cosmic ray, low-energy charged particle and magnetometer instruments, with some additional charged particle data obtained through April of this year.

Voyager 2 is about 9 billion miles (15 billion kilometers) from the sun and still inside the heliosphere. Voyager 1 was about 11 billion miles (18 billion kilometers) from the sun Aug. 25 when it reached the magnetic highway, also known as the depletion region, and a connection to interstellar space. This region allows charged particles to travel into and out of the heliosphere along a smooth magnetic field line, instead of bouncing around in all directions as if trapped on local roads. For the first time in this region, scientists could detect low-energy cosmic rays that originate from dying stars.

"We saw a dramatic and rapid disappearance of the solar-originating particles. They decreased in intensity by more than 1,000 times, as if there was a huge vacuum pump at the entrance ramp onto the magnetic highway," said Stamatios Krimigis, the low-energy charged particle instrument's principal investigator at the Johns Hopkins University Applied Physics Laboratory in Laurel, Md. "We have never witnessed such a decrease before, except when Voyager 1 exited the giant magnetosphere of Jupiter, some 34 years ago."

Other charged particle behavior observed by Voyager 1 also indicates the spacecraft still is in a region of transition to the interstellar medium. While crossing into the new region, the charged particles originating from the heliosphere that decreased most quickly were those shooting straightest along solar magnetic field lines. Particles moving perpendicular to the magnetic field did not decrease as quickly. However, cosmic rays moving along the field lines in the magnetic highway region were somewhat more populous than those moving perpendicular to the field. In interstellar space, the direction of the moving charged particles is not expected to matter.

In the span of about 24 hours, the magnetic field originating from the sun also began piling up, like cars backed up on a freeway exit ramp. But scientists were able to quantify that the magnetic field barely changed direction -- by no more than 2 degrees.

"A day made such a difference in this region with the magnetic field suddenly doubling and becoming extraordinarily smooth," said Leonard Burlaga, the lead author of one of the papers, and based at NASA's Goddard Space Flight Center in Greenbelt, Md. "But since there was no significant change in the magnetic field direction, we're still observing the field lines originating at the sun."

NASA's Jet Propulsion Laboratory, in Pasadena, Calif., built and operates the Voyager spacecraft. California Institute of Technology in Pasadena manages JPL for NASA. The Voyager missions are a part of NASA's Heliophysics System Observatory, sponsored by the Heliophysics Division of the Science Mission Directorate at NASA Headquarters in Washington.

For more information about the Voyager spacecraft mission, visit: http://www.nasa.gov/voyager and http://voyager.jpl.nasa.gov .

Media contact:

Jia-Rui C. Cook 818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif.
jccook@jpl.nasa.gov

Steve Cole 202-358-0918
NASA Headquarters, Washington
stephen.e.cole@nasa.gov

2013-209

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Trailblazer Sea Satellite Marks its Coral Anniversary

JPL/NASA News
News feature: 2013-208                                                                       June 27, 2013

Trailblazer Sea Satellite Marks its Coral Anniversary

Artist's concept of Seasat

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.php?release=2013-208&cid=release_2013-208

"The true worth of a man is not to be found in man himself, but in the colours and textures that come alive in others."

- Albert Schweitzer

History tends to look fondly upon trailblazers, even if they don't necessarily stick around. From musicians and actors to politicians and inventors, our lives are immeasurably enriched by the contributions of visionaries who left us.

So when NASA's Jet Propulsion Laboratory, Pasadena, Calif., launched an experimental satellite called Seasat to study Earth and its seas 35 years ago this week, only to see the mission end just 106 days later due to an unexpected malfunction, some at the time may have looked upon it as a failure. But this spunky satellite, which is still in orbit, shining in the night sky at magnitude 4.0, continues to live on through the many Earth and space observation missions it has spawned.

Seasat's tale began in 1969, when a group of engineers and scientists from multiple institutions convened at a conference in Williamstown, Mass., to study how satellites could be used to improve our understanding of the ocean. Three years later, NASA began planning for Seasat, the first multi-sensor spacecraft dedicated specifically to observing Earth's ocean. A broad user working group from many organizations defined its requirements. JPL was selected to manage the project, and numerous other NASA centers and government and industry partners participated. On the night of June 26, 1978, Seasat was launched from California's Vandenberg Air Force Base aboard an Atlas-Agena rocket, carrying with it three prototype radar instruments and two radiometers.

During its brief life, Seasat collected more information about ocean physics than had been acquired in the previous 100 years of shipboard research. It established satellite oceanography and proved the viability of several radar sensors, including an imaging radar, for studying our planet. Most importantly, it spawned many subsequent Earth remote-sensing satellites and instruments at JPL and elsewhere that track changes in Earth's ocean, land and ice, including many currently in orbit or in development. Its advances were also subsequently applied to missions to study other planets.

Post-Seasat NASA program manager Stan Wilson said Seasat demonstrated the potential usefulness of ocean microwave observations. "As a result, at least 50 satellites have been launched by more than a dozen space agencies to carry microwave instruments to observe the ocean. In addition, we have two continuing records of critical climate change in the ocean that are impacting society today: diminishing ice cover in the Arctic and rising global sea level. What greater legacy could a mission have?"

"Seasat flew long enough to fully demonstrate its groundbreaking remote sensing technologies, and its early death permitted the limited available resources to be marshaled toward processing and analyzing its approximately 100-day data set," said Bill Townsend, Seasat radar altimeter experiment manager. "This led to other systems, both nationally and internationally, that continued Seasat's legacy, enabling Seasat technologies to be used to better understand climate change."

Seasat's experimental instruments included a synthetic aperture radar (SAR), which provided the first-ever highly detailed radar images of ocean and land surfaces from space; a radar scatterometer, which measured near-surface wind speed and direction; a radar altimeter, which measured ocean surface height, wind speed and wave heights; and a scanning multichannel microwave radiometer that measured atmospheric and ocean data, including wind speeds, sea ice cover, atmospheric water vapor and precipitation, and sea surface temperatures in both clear and cloudy conditions.

On June 28, the Alaska Satellite Facility will release newly processed digital SAR imagery from Seasat. The imagery, available for download at http://www.asf.alaska.edu , will enable scientists to travel back in time to research the ocean, sea ice, volcanoes, forests, land cover, glaciers and more. Before now, only about 20 percent of Seasat SAR data had been processed digitally.

In oceanography, Seasat gave us our first global view of ocean circulation, waves and winds, providing new insights into the links between the ocean and atmosphere that drive our climate. For the first time, the state of an entire ocean could be seen all at once. Seasat's altimeter, which used pulses of microwave radiation to measure the distance from the satellite to the ocean surface precisely, mapped ocean surface topography, allowing scientists to demonstrate how sea surface conditions could be used to determine ocean circulation and heat storage. The data also revealed new information about Earth's gravity field and the topography of the ocean floor.

"The short 100-day Seasat mission provided a moment of epiphany to remind people that the vast ocean is best accessed from space," said Lee-Lueng Fu, JPL senior research scientist and project scientist for the NASA/French Space Agency Jason-1 satellite and NASA's planned Surface Water and Ocean Topography mission.

Seasat inspired a whole generation of scientists. "I decided to take a job offer at JPL fresh out of graduate school because I was told that the future of oceanography is in satellite oceanography and the future of satellite oceanography will begin with Seasat at JPL," said JPL oceanographer Tim Liu. "I did not plan to stay forever, but I have now been here more than three decades."

Since Seasat, advanced ocean altimeters on the NASA/European Topex/Poseidon and Jason missions have been making precise measurements of sea surface height used to study climate phenomena such as El Niño and La Niña. The newest Jason mission, Jason-3, is scheduled to launch in 2015 to continue the 20-plus-year climate data record. Satellite altimetry has been used to improve weather and climate models, ship routing, marine mammal studies, fisheries management and offshore operations. Seasat's scatterometer gave us our first real-time global map of the speed and direction of ocean winds, which drive waves and currents and are the major link between the ocean and atmosphere. A scatterometer is a microwave radar sensor used to measure the reflection or scattering effect produced while scanning the surface of Earth from an aircraft or a satellite. The technology was later used on JPL's NASA Scatterometer, Quikscat spacecraft, SeaWinds instrument on Japan's Midori 2 spacecraft and the OSCAT instrument on India's Oceansat-2. It will also be used on JPL's ISS-RapidScat instrument, launching to the International Space Station in the spring of 2014. Data from these scatterometers, including three scatterometers launched by the European Space Agency, help forecasters predict hurricanes, tropical storms and El Ninos.

Seasat's microwave radiometer, which subsequently flew on NASA's Nimbus-7 satellite, led to numerous successful radiometer instruments and missions used for oceanography, weather and climate research. Radiometers measure particular wavelengths of microwave energy. The Seasat radiometer's heritage includes the Special Sensor Microwave Imager instruments launched on United States Air Force Defense Meteorological Satellite Program satellites, the joint NASA/Japanese Aerospace Exploration Agency (JAXA) Tropical Rainfall Measuring Mission microwave imager, the Advanced Microwave Scanning Radiometer (AMSR)-E that flew aboard NASA's Aqua spacecraft, JAXA's current AMSR-2 instrument, and numerous other radiometers launched by Europe, China and India. The radiometer, scatterometer and SAR for NASA's Soil Moisture Active Passive mission to measure global soil moisture, launching in 2014, also draw upon Seasat's heritage.

By simultaneously flying a radiometer with a radar altimeter, Seasat demonstrated the benefit of using radiometer measurements of water vapor to correct altimeter measurements of sea surface height. Water vapor affects the accuracy of altimeter measurements by delaying the time it takes for the altimeter's signals to make their round trip to the ocean surface and back. This technique has been used on all subsequent NASA/European satellite altimetry missions.

Seasat's oceanographic mission also studied sea ice and its role in controlling Earth's climate. Its SAR provided the first high-resolution images of sea ice, measuring its movement, deformation and age. Today, SAR and scatterometers are also used to monitor Earth's ice from space.

"It's hard to imagine where we would be without the radiometer pioneered on Seasat, but certainly much further behind in critical Earth observations than we are now," said Gary Lagerloef of Earth & Space Research, Seattle, principal investigator of NASA's Aquarius mission to map ocean surface salinity. The Aquarius radiometer and scatterometer also trace their heritage back to Seasat.

Seasat's SAR monitored the global surface wave field and revealed many oceanic- and atmospheric-related phenomena, from current boundaries to eddies and internal waves.

Beyond the ocean, Seasat's SAR provided spectacular images of Earth's land surfaces and geology. Seasat data were used to pioneer radar interferometry, which uses microwave energy pulses sent from sensors on satellites or aircraft to the ground to detect land surface changes such as those created by earthquakes, and measure land surface topography. Three JPL Shuttle Imaging Radar experiments flew on the Space Shuttle in the 1980s/1990s. In 2000, JPL's Shuttle Radar Topography Mission used the technology to create the world's most detailed topographic measurements of more than 80 percent of Earth's land surface. Today, the technology is being used on JPL's Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR) airborne imaging radar system for a wide variety of Earth studies. Among the international SAR missions with heritages tracing to Seasat are the Japanese Earth Resources Satellite 1 and Advanced Land Observing System 1, the Canadian/U.S. Radarsat 1 and the European Space Agency's Remote Sensing Satellites. The technology will also be used on NASA's planned Surface Water and Ocean Topography mission, planned for launch in 2020.

Paul Rosen, JPL project scientist for a future NASA L-band SAR spacecraft currently under study, said Seasat's demonstration of spaceborne repeat-pass radar interferometry to measure minute Earth surface motions has led to a new field of space geodetic imaging and forms the basis for his new mission.

"Together with international L-band SAR sensors, we have the opportunity in the next five years to create a 40-year observation record of land-use change where overlapping observations exist," Rosen said. "These time-lapse images of change will provide fascinating insights into urban growth, agricultural patterns and other signs of human-induced changes over decades and climate change in the polar regions."

Beyond Earth, Seasat technology was used on JPL's Magellan mission, which mapped 99 percent of the previously hidden surface of Venus, and the Titan radar onboard the JPL-built and -managed Cassini orbiter to Saturn.

Seasat was managed by JPL for NASA, with significant participation from NASA's Goddard Space Flight Center, Greenbelt, Md.; NASA's Wallops Flight Facility, Wallops Island, Va.; NASA's Langley Research Center, Hampton, Va.; NASA's Glenn Research Center, Cleveland, Ohio; Johns Hopkins University Applied Physics Laboratory, Laurel, Md.; Lockheed Missiles and Space Systems, Sunnyvale, Calif.; and NOAA, Washington, D.C.

For more on Seasat, visit: http://podaac.jpl.nasa.gov/SeaSAT and http://www.jpl.nasa.gov/multimedia/seasat/intro.html . JPL is a division of the California Institute of Technology, Pasadena.

Media contact:

Alan Buis
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-0474
alan.buis@jpl.nasa.gov

2013-208

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ScienceDaily: Extrasolar Planets News

ScienceDaily: Extrasolar Planets News


First transiting planets in a star cluster discovered

Posted: 26 Jun 2013 01:28 PM PDT

All stars begin their lives in groups. Most stars are born in small groups that quickly fall apart. Others form in huge, dense swarms, where stars jostle with thousands of neighbors while strong radiation and harsh stellar winds scour interstellar space, stripping planet-forming materials from nearby stars. It would thus seem an unlikely place to find alien worlds. Yet 3,000 light-years from Earth, in the star cluster NGC 6811, astronomers have found two planets smaller than Neptune orbiting sun-like stars.

Survivor of stellar collision is new type of pulsating star

Posted: 26 Jun 2013 11:28 AM PDT

Astronomers have observed the remnant of a stellar collision and discovered that its brightness varies in a way not seen before on this rare type of star. By analyzing the patterns in these brightness variations, astronomers will learn what really happens when stars collide.

ScienceDaily: Astronomy News

ScienceDaily: Astronomy News


First transiting planets in a star cluster discovered

Posted: 26 Jun 2013 01:28 PM PDT

All stars begin their lives in groups. Most stars are born in small groups that quickly fall apart. Others form in huge, dense swarms, where stars jostle with thousands of neighbors while strong radiation and harsh stellar winds scour interstellar space, stripping planet-forming materials from nearby stars. It would thus seem an unlikely place to find alien worlds. Yet 3,000 light-years from Earth, in the star cluster NGC 6811, astronomers have found two planets smaller than Neptune orbiting sun-like stars.

Astronomers spy on galaxies in the raw

Posted: 26 Jun 2013 08:36 AM PDT

A radio telescope has detected the raw material for making the first stars in galaxies that formed when the Universe was just three billion years old -- less than a quarter of its current age.

ScienceDaily: Galaxies News

ScienceDaily: Galaxies News


Astronomers spy on galaxies in the raw

Posted: 26 Jun 2013 08:36 AM PDT

A radio telescope has detected the raw material for making the first stars in galaxies that formed when the Universe was just three billion years old -- less than a quarter of its current age.

ScienceDaily: Stars News

ScienceDaily: Stars News


First transiting planets in a star cluster discovered

Posted: 26 Jun 2013 01:28 PM PDT

All stars begin their lives in groups. Most stars are born in small groups that quickly fall apart. Others form in huge, dense swarms, where stars jostle with thousands of neighbors while strong radiation and harsh stellar winds scour interstellar space, stripping planet-forming materials from nearby stars. It would thus seem an unlikely place to find alien worlds. Yet 3,000 light-years from Earth, in the star cluster NGC 6811, astronomers have found two planets smaller than Neptune orbiting sun-like stars.

Survivor of stellar collision is new type of pulsating star

Posted: 26 Jun 2013 11:28 AM PDT

Astronomers have observed the remnant of a stellar collision and discovered that its brightness varies in a way not seen before on this rare type of star. By analyzing the patterns in these brightness variations, astronomers will learn what really happens when stars collide.

Astronomers spy on galaxies in the raw

Posted: 26 Jun 2013 08:36 AM PDT

A radio telescope has detected the raw material for making the first stars in galaxies that formed when the Universe was just three billion years old -- less than a quarter of its current age.

Wednesday, June 26, 2013

ScienceDaily: Stars News

ScienceDaily: Stars News


Three planets in habitable zone of nearby star: Gliese 667c reexamined

Posted: 25 Jun 2013 04:35 AM PDT

Astronomers have combined new observations of Gliese 667C with existing data to reveal a system with at least six planets. A record-breaking three of these planets are super-Earths lying in the zone around the star where liquid water could exist, making them possible candidates for the presence of life. This is the first system found with a fully packed habitable zone.

ScienceDaily: Extrasolar Planets News

ScienceDaily: Extrasolar Planets News


Three planets in habitable zone of nearby star: Gliese 667c reexamined

Posted: 25 Jun 2013 04:35 AM PDT

Astronomers have combined new observations of Gliese 667C with existing data to reveal a system with at least six planets. A record-breaking three of these planets are super-Earths lying in the zone around the star where liquid water could exist, making them possible candidates for the presence of life. This is the first system found with a fully packed habitable zone.

ScienceDaily: Astronomy News

ScienceDaily: Astronomy News


Three planets in habitable zone of nearby star: Gliese 667c reexamined

Posted: 25 Jun 2013 04:35 AM PDT

Astronomers have combined new observations of Gliese 667C with existing data to reveal a system with at least six planets. A record-breaking three of these planets are super-Earths lying in the zone around the star where liquid water could exist, making them possible candidates for the presence of life. This is the first system found with a fully packed habitable zone.

Tuesday, June 25, 2013

ScienceDaily: Astronomy News

ScienceDaily: Astronomy News


Five years of stereo imaging for NASA's TWINS

Posted: 24 Jun 2013 11:16 AM PDT

Surrounding Earth is a dynamic region called the magnetosphere. The region is governed by magnetic and electric forces, incoming energy and material from the sun, and a vast zoo of waves and processes unlike what is normally experienced in Earth-bound physics. Nestled inside this constantly changing magnetic bubble lies a donut of charged particles generally aligned with Earth's equator. Known as the ring current, its waxing and waning is a crucial part of the space weather surrounding our planet, able to induce magnetic fluctuations on the ground as well as to transmit disruptive surface charges onto spacecraft.

Messier 61 looks straight into Hubble's camera

Posted: 24 Jun 2013 11:13 AM PDT

The NASA/ESA Hubble Space Telescope has captured a new image of nearby spiral galaxy Messier 61, also known as NGC 4303. The galaxy, located only 55 million light-years away from Earth, is roughly the size of the Milky Way, with a diameter of around 100,000 light-years.

Billion-pixel view of Mars comes from Curiosity rover

Posted: 24 Jun 2013 10:52 AM PDT

A billion-pixel view from the surface of Mars, from NASA's Mars rover Curiosity, offers armchair explorers a way to examine one part of the Red Planet in great detail.

Mystery of the gigantic storm on Saturn

Posted: 24 Jun 2013 04:57 AM PDT

We now understand the nature of the giant storms on Saturn. Through the analysis of images as well as the computer models of the storms and the examination of the clouds therein, astronomers have managed to explain the behavior of these storms for the very first time.