Monday, February 08, 2010

Radar Studies Continue in Hispaniola

NASA radar imaging flights over Central America, Haiti and the Dominican Republic are in the second week of a three-week campaign.

The JPL-developed Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR) is currently in the second week of a three-week campaign in Central America, Haiti and the Dominican Republic. Flying beneath the belly of a modified Gulfstream III aircraft from NASA’s Dryden Flight Research Center, the sophisticated radar can spot minute changes in Earth's surface by flying precise repeat passes over targeted areas.

The Central American survey flights are focusing on measuring biomass in Central American rain forests, imaging volcanoes from Guatemala to Costa Rica, and imaging Mayan ruins. The flights over Haiti and the Dominican Republic are targeting earthquake faults on the island of Hispaniola. Scientists collected data over Central American nations again on Feb. 2, and then flew a second set of data tracks over Haiti on Feb. 3 before returning to Costa Rica on Feb. 4.

Wednesday, February 03, 2010

Envisioning Future Flight

Today's students will be designing tomorrow's aircraft, and NASA's Fundamental Aeronautics Student Competition gives them a head start.

Each year, the competition challenges students to research a particular real-world issue in aeronautics and to develop their own solutions to the problem.

Past participants in NASA's Fundamental Aeronautics Student Competition said the experience was a rewarding one that helped them learn more about aeronautics and encouraged them to improve their approaches to research and creative problem-solving.

In the 2008-2009 competition, students were challenged to develop ideas for making commercial supersonic air transportation available by 2020. Contest participants did so by examining obstacles to supersonic transportation and proposing solutions. In an additional challenge, some students submitted designs for a small supersonic airliner.

Thursday, January 28, 2010

Cassini's Next Look at Titan

Sixteen days after last visiting Saturn's largest moon, NASA's Cassini spacecraft returns for another look-see of the cloud-shrouded moon - this time from on high. The flyby on Thursday, Jan. 28, referred to as "T-66" in the hollowed halls of Cassini operations, will place the spacecraft within 7,490 kilometers (4,654 miles) above the surface during time of closest approach.

While this latest close approach places Cassini more than 6,400 kilometers (3,970 miles) higher above Titan's surface than the Jan. 12 flyby, it should not considered of lesser scientific value. Instead, this high-altitude encounter will provide an opportunity for some of the spacecraft's instruments to gain another unique perspective on this crepuscular world.

Monday, January 25, 2010

First of Many Asteroid Finds

The red dot at the center of this image is the first near-Earth asteroid discovered by NASA's Wide-Field Infrared Survey Explorer, or WISE -- an all-sky mapping infrared mission designed to see all sorts of cosmic objects.

Near-Earth objects are asteroids and comets with orbits that come close to Earth's path around the sun. This particular asteroid, called 2010 AB78, is roughly one kilometer (0.6 miles) in diameter, and is currently about 158 million kilometers (98 million miles) away from Earth. Its elliptical-shaped orbit takes it out beyond Mars and back in about as close to the sun as Earth. Because the asteroid's orbit is tilted relative to the plane of our solar system, astronomers do not think it poses a hazard to our planet. As with all near-Earth objects, 2010 AB78 will continue to be monitored.

The image shows three infrared wavelengths, with red representing the longest wavelength of 12 microns, and green and blue showing 4.6- and 3.4-micron light, respectively. The asteroid appears redder than the rest of the background stars because it is cooler and emits most of its light at longer infrared wavelengths. In visible light, this space rock is very faint and difficult to see.

WISE, which began its all-sky survey on Jan. 14, 2010, is expected to find about one hundred thousand previously undiscovered asteroids in the Main Belt between Mars and Jupiter, and hundreds of new near-Earth asteroids. It will also spot millions of new stars and galaxies.

Thursday, January 21, 2010

Rover Gives NASA an "Opportunity" to View Interior of Mars

NASA's Mars Exploration Rover Opportunity examined a rock called "Marquette Island" from mid-November 2009 until mid-January 2010. Studies of texture and composition suggest that this rock, not much bigger than a basketball, originated deep inside the Martian crust. A crater-digging impact could have excavated the rock and thrown it a long distance, to where Opportunity found it along the rover's long trek across the Meridiani plain toward Endeavour Crater.

This approximately true-color view of Marquette Island comes from combining three exposures that Opportunity's panoramic camera (Pancam) took through different filters during the rover's 2,117th Martian day, or sol, on Mars (Jan. 6, 2010). On the preceding sol, Opportunity's rock abrasion tool brushed dust out of the circular area where that tool had ground into the rock on sols 2100 and 2103 (Dec. 20 and 23, 2009). The dark circle left by the rock abrasion tool's work is approximately 5 centimeters (2 inches) in diameter.

Second Warmest Year on Record; End of Warmest Decade

2009 was tied for the second warmest year in the modern record, a new NASA analysis of global surface temperature shows. The analysis, conducted by the Goddard Institute for Space Studies (GISS) in New York City, also shows that in the Southern Hemisphere, 2009 was the warmest year since modern records began in 1880.

Although 2008 was the coolest year of the decade -- due to strong cooling of the tropical Pacific Ocean -- 2009 saw a return to near-record global temperatures. The past year was only a fraction of a degree cooler than 2005, the warmest year on record, and tied with a cluster of other years --1998, 2002, 2003, 2006 and 2007 1998 and 2007 -- as the second warmest year since recordkeeping began.

“There’s always an interest in the annual temperature numbers and on a given year’s ranking, but usually that misses the point,” said James Hansen, the director of GISS. “There's substantial year-to-year variability of global temperature caused by the tropical El Niño-La Niña cycle. But when we average temperature over five or ten years to minimize that variability, we find that global warming is continuing unabated."

Monday, January 18, 2010

Endeavour's STS-130 Mission


Commander George Zamka will lead the STS-130 mission to the International Space Station aboard space shuttle Endeavour. Terry Virts will serve as the pilot. Mission Specialists are Nicholas Patrick, Robert Behnken, Stephen Robinson and Kathryn Hire. Virts will be making his first trip to space.

Shuttle Endeavour and its crew will deliver to the space station a third connecting module, the Italian-built Tranquility node and the seven-windowed cupola, which will be used as a control room for robotics. The mission will feature three spacewalks.

Liftoff from NASA's Kennedy Space Center in Florida is targeted for February 7, 2010, at 4:39 a.m. EST

Tuesday, January 12, 2010

Solar Scientists Use 'Magnetic Mirror Effect' to Reproduce IBEX Observation



Ever since NASA's Interstellar Boundary Explorer, or IBEX, mission scientists released the first comprehensive sky map of our solar system's edge in particles, solar physicists have been busy revising their models to account for the discovery of a narrow "ribbon" of bright emission that was completely unexpected and not predicted by any model at the time.

Further study by a team of scientists funded through NASA's Heliophysics Guest Investigator program has produced a revised model that explains and closely reproduces the IBEX result by incorporating a single new effect into an existing model. The new effect, put forward by the IBEX team soon after sighting of the ribbon, is that the magnetic field surrounding our solar system—called the local galactic magnetic field—acts like a mirror for the particles that IBEX sees.