This dazzling image shows the globular cluster Messier 69, or M 69 for short, as viewed through the NASA/ESA Hubble Space Telescope. Globular clusters are dense collections of old stars. In this picture, foreground stars look big and golden when set against the backdrop of the thousands of white, silvery stars that make up M 69.

Another aspect of M 69 lends itself to the bejeweled metaphor: As globular clusters go, M 69 is one of the most metal-rich on record. In astronomy, the term "metal" has a specialized meaning: it refers to any element heavier than the two most common elements in our Universe, hydrogen and helium. The nuclear fusion that powers stars created all of the metallic elements in nature, from the calcium in our bones to the carbon in diamonds. Successive generations of stars have built up the metallic abundances we see today.

Because the stars in globular clusters are ancient, their metallic abundances are much lower than more recently formed stars, such as the Sun. Studying the makeup of stars in globular clusters like M 69 has helped astronomers trace back the evolution of the cosmos.

M 69 is located 29 700 light-years away in the constellation Sagittarius (the Archer). The famed French comet hunter Charles Messier added M 69 to his catalogue in 1780. It is also known as NGC 6637.

The image is a combination of exposures taken in visible and near-infrared light by Hubble’s Advanced Camera for Surveys, and covers a field of view of approximately 3.4 by 3.4 arcminutes.

Read more

Hubble Catches Glowing Gas and Dark Dust in a Side-On Spiral

The NASA/ESA Hubble Space Telescope has produced a sharp image of NGC 4634, a spiral galaxy seen exactly side-on. Its disk is slightly warped by ongoing interactions with a nearby galaxy, and it is crisscrossed by clearly defined dust lanes and bright nebulae.

NGC 4634, which lies around 70 million light-years from Earth in the constellation of Coma Berenices, is one of a pair of interacting galaxies. Its neighbor, NGC 4633, lies just outside the upper right corner of the frame, and is visible in wide-field views of the galaxy. While it may be out of sight, it is not out of mind: its subtle effects on NGC 4634 are easy to see to a well-trained eye.

Gravitational interactions pull the neat spiral forms of galaxies out of shape as they get closer to each other, and the disruption to gas clouds triggers vigorous episodes of star formation. While this galaxy’s spiral pattern is not directly visible thanks to our side-on perspective, its disk is slightly warped, and there is clear evidence of star formation.

Along the full length of the galaxy, and scattered around parts of its halo, are bright pink nebulae. Similar to the Orion Nebula in the Milky Way, these are clouds of gas that are gradually coalescing into stars. The powerful radiation from the stars excites the gas and makes it light up, much like a fluorescent sign. The large number of these star formation regions is a telltale sign of gravitational interaction.

Read more

NASA's Ocean Salinity Pathfinder Celebrates its First Year in Orbit

It's been a busy first year in space for Aquarius, NASA's pioneering instrument to measure ocean surface salinity from orbit.

Designed to advance our understanding of what changes in the saltiness of the ocean's top layer say about the water cycle and variations in climate, Aquarius took only two and a half months after its launch to start measuring global salinity patterns. Since then, it has also observed regional features such as the freshwater plume gushing from the Amazon River and localized changes in ocean saltiness following a tropical storm.

"It was a very remarkable achievement, that within such a short period of time after turning the instrument on we were producing very good-looking data," said Aquarius Principal Investigator Gary Lagerloef, of Earth & Space Research in Seattle. "It was beyond our expectations."

Lagerloef said that objectives for Aquarius' second year in orbit include correcting a few remaining calibration errors and validating the Aquarius dataset with thousands of direct in-water measurements of salinity.

The Aquarius/Satélite de Aplicaciones Científicas (SAC)-D mission is an international collaboration of NASA and Argentina's space agency. The satellite also carries instruments from partner institutions in Canada, Italy and France.

A Delta II rocket carrying the international observatory launched from Vandenberg Air Force Base in California, on June 10, 2011. Less than an hour later, the satellite separated from the rocket, started its deployment and established communications with ground stations.

"The first time the thing chirped, we got the data and posted it on the Web. It was just basic telemetry at that point, but it showed that all the systems we had put in place to share the data worked," said Gene Feldman, Aquarius project manager at NASA Goddard Space Flight Center in Greenbelt, Md. "We didn't get to pop champagne – we didn't have the time!"

Aquarius is the first NASA instrument specifically designed to study superficial ocean salinity from space, and it does it at a rate of about 300,000 measurements per month. It uses three passive microwave sensors, called radiometers, to record the thermal signal from the oceans' top 0.4 inches (10.1 millimeters). This signal varies depending on the concentration of salt and the temperature of the waters.

"An overarching question in climate research is to understand how changes in the Earth's water cycle – meaning rainfall and evaporation, river discharges and so forth – ocean circulation, and climate link together," Lagerloef said. Most global precipitation and evaporation events take place over the ocean and are very difficult to measure. But rainfall freshens the oceans' surface waters, and Aquarius can detect these changes in saltiness. "Salinity is the variable we can use to measure that coupling effect. It's a critical factor and it will eventually be used to improve climate forecast models."

Aquarius became operational on Aug. 25, 2011. The project's scientists soon created a map of global ocean saltiness using the first two and a half weeks of measurements, which had been compared against reference salinity data. The map showed variations in salinity patterns in much greater detail than Aquarius researchers had expected to see so early in the mission. Another welcome surprise was the observation of the effects on the ocean of Tropical Storm Lee (Sept. 2-3, 2011). Heavy rains produced a low-salinity feature that lasted more than a month in the Gulf of Mexico between the Mississippi River delta and the Florida panhandle.

Read more

Beaming Success for Station Fans

Did you ever use a flashlight to send a Morse code message to your neighbor at night as a kid? People like to say hello using lights and it's no different for space aficionados who want to twinkle a greeting from the Earth to the International Space Station during a sighting as it passes overhead -- except that it is a whole lot more complicated.

Although the space station has been in orbit for more than a decade, the first successful flashing of a beam of light to the laboratory happened only recently. On March 3, 2012, the San Antonio Astronomical Association met to attempt to shine a signal to the station. Aboard the orbiting lab, astronaut Don Pettit was watching and waiting.

"It sounds deceptively easy," said Pettit in a related blog entry. "But like so many other tasks, it becomes much more involved in the execution than in the planning."

The ground group used a one-watt blue laser and a white spotlight to track the station as it flew overhead. Pettit worked via e-mail with the association members to run complicated engineering calculations to ensure they were accurately tracking the station. Considerations included the diameter of the light beam, the intensity of the laser, and the fact that the station is a moving target, as Pettit pointed out in another blog post on the difficulty of Earth photography from space.

"From my orbital perspective, I am sitting still and Earth is moving," said Pettit. "I sit above the grandest of all globes spinning below my feet, and watch the world speed by at an amazing eight kilometers per second [approximately 17,880 miles per hour]."

Pettit had additional complications to address to capture an image of the beam of light from the Texas fans of the space station. Even with a shutter speed of 1/1000 of a second, the camera he used on station was not fast enough to photograph the Earth below, which also is moving. To compensate for this, Pettit used precise manual tracking -- a technique of moving the camera along the same path as the object being photographed -- a skill perfected on orbit while working on Crew Earth Observations research.

While photographing the Earth may provide an entertaining pastime for the crew, there also are important research goals and benefits for those of us on the ground. It can take up to a month, according to Pettit, for astronauts to become proficient at taking this kind of planned image. The crew's photographic efforts can provide orbital perspectives of natural disasters and man-made alterations of the planet, which aid in relief and environmental efforts.

Preparing to capture the laser flash provided practice for Pettit in planning and tracking a specific Earth target. With the station circling the Earth every 90 minutes, you might think there is ample opportunity, but the circumstances of the pass had to align. Pettit and the team in San Antonio had to choose their timing carefully, selecting a "dark pass" when the station could see the ground, but those on the ground could not see the station.

"Ironically, when earthlings can see us, we cannot see them," said Pettit. "The glare from the full sun effectively turns our windows into mirrors that return our own ghostly reflection. This often plays out when friends want to flash space station from the ground as it travels overhead."

Read more

Having a Solar Blast

The Sun unleashed an M-2 (medium-sized) solar flare, an S1-class (minor) radiation storm and a spectacular coronal mass ejection (CME) on June 7, 2011 from sunspot complex 1226-1227. The large cloud of particles mushroomed up and fell back down looking as if it covered an area of almost half the solar surface.

The Solar Dynamics Observatory (SDO) observed the flare's peak at 1:41a.m. ET (0641 UT). SDO recorded these images (above) in extreme ultraviolet light that show a very large eruption of cool gas. It is somewhat unique because at many places in the eruption there seems to be even cooler material -- at temperatures less than 80,000 K. All of the solar Heliophysics System Observatory missions captured the event.

When viewed in Solar and Heliospheric Observatory's (SOHO) coronagraphs (top right), the event shows bright plasma and high-energy particles roaring from the Sun.

Also to the right are links to the Solar Terrestrial Relations Observatory (STEREO) Ahead and Behind coronograph videos showing the CME expansion as viewed from each side of the sun. The STEREO Ahead satellite precedes the Earth as it circles the Sun. The STEREO Behind satellite follows behind the Earth in it's orbit of the Sun.

This not-squarely Earth-directed CME is moving at 1400 km/s according to NASA models. The CME should deliver a glancing blow to Earth's magnetic field during the late hours of June 8th or June 9th. High-latitude sky watchers should be alert for auroras when the CME arrives.

NASA Satellite Data Reveals Joplin Tornado Track

The image shows the Advanced Spaceborne Thermal Emission and Reflection Radiometer, or ASTER, satellite data acquired on May 30, 2011, showing the damage track resulting from for the EF-5 tornado associated with the May 22, 2011, Joplin, Mo. storm. The complex pattern of ASTER data indicate variability in land use characterized by colors in this three-channel composite. Vegetated areas are shown in red and green, urban areas are aqua and the damage track from the tornado is also aqua. Clouds are white and cloud shadows are dark in color. The ASTER data here shows the tornado damage scar, aqua in color, left by the violent tornado as damage disrupts other, more typical land use patterns. The variation in width is likely correlated to tornado intensity. The tornado abruptly moved in a more southeasterly direction to the east of the city as is somewhat apparent through the clouds in the ASTER imagery.

This image was created by the NASA Short-term Prediction Research and Transition, or SPoRT, Center at Marshall Space Flight Center in Huntsville, Ala., using ASTER data provided courtesy of NASA's Goddard Space Flight Center in Greenbelt, Md.; the United States Geological Survey Land Processes Distributed Active Archive Center in Sioux Falls, S.D.; Japan’s Earth Remote Sensing Data Analysis Center in Tokyo, Japan; the Ministry of Economy, Trade and Industry, along with the Japan Research Observation System Organization. Final ASTER imagery was produced using resources of the Nebula Cloud Computing Platform, tiled, and displayed within Google Earth. Storm survey information was provided by the National Weather Service Forecast Office in Springfield, Mo.

Last Female Shuttle Astronaut Available For Interviews

NASA astronaut Sandra Magnus, who will fly on the last space shuttle mission next month, is available for live satellite interviews from 7 to 9 a.m. CDT on Monday, June 6. Shuttle Atlantis is targeted to launch July 8 with Magnus, Commander Chris Ferguson, Pilot Doug Hurley and Mission Specialist Rex Walheim to deliver supplies and spare equipment to the International Space Station.After her first spaceflight in 2002, Magnus became the 34th out of 47 woman to fly aboard the shuttle, which launched the first American woman into space, Sally Ride, in 1983. With the upcoming STS-135 launch, Magnus will be the last female astronaut to fly on the storied vehicle.

Magnus is a native of Belleville, Ill. She earned a bachelor's and a master's from the University of Missouri-Rolla and a doctorate from the Georgia Institute of Technology.She is a veteran of two shuttle flights and a 4.5-month stay aboard the station as a member of the Expedition 18 crew. Her first spaceflight was aboard shuttle Atlantis on the STS-112 mission in October 2002. She later flew to the station aboard shuttle Endeavour on STS-126 in November 2008 and returned to Earth aboard shuttle Discovery on STS-119 in March 2009.

To arrange an interview, news media representatives must contact Karen Svetaka at 281-483-8684, no later than 4 p.m. on Friday, June 3. Participating media must tune into NASA Television's Live Interview Media Outlet channel. The channel is a digital satellite C-band downlink by uplink provider Americom.It is on satellite AMC 3, transponder 9C, located at 87 degrees west, downlink frequency 3865.5 MHz based on a standard C-band, horizontal downlink polarity. FEC is 3/4, data rate is 6.0 Mbps, symbol rate is 4.3404 Msps, transmission DVB-S, 4:2:0. NASA TV will air the Magnus interviews live. Video b-roll of STS-135 flight preparations will air June 6 at 6:30 a.m

Space Shuttle Endeavour Returns to Earth for Final Time Wednesday

Space shuttle Endeavour is scheduled to return to Earth for the final time on Wednesday, June 1, completing a 16-day mission to outfit the International Space Station. If Endeavour lands Wednesday, it will have spent 299 days in space and traveled more than 122.8 million miles during its 25 flights. It launched on its first mission on May 7, 1992.Wednesday's landing opportunities at NASA's Kennedy Space Center in Florida are at 2:35 a.m. and 4:11 a.m. EDT. Endeavour's entry flight control team led by Tony Ceccacci will evaluate weather conditions at Kennedy before permitting Endeavour to land.
If the shuttle is unable to return Wednesday, additional opportunities are available on Thursday at Kennedy and at backup landing site Edwards Air Force Base in California. For recorded updates about landing, call 321-867-2525.Approximately two hours after Endeavour lands, NASA officials will hold a briefing to discuss the mission. The participants will be:

• Bill Gerstenmaier, associate administrator for Space Operations


• Mike Moses, space shuttle launch integration manager


• Mike Leinbach, space shuttle launch director

After touchdown, the astronauts will undergo routine physical examinations and meet with their families. The crew is expected to participate in a post-landing news conference about six hours after landing. Availability is subject to change due to real time circumstances. The news events will be broadcast live on NASA Television and the agency's website.

The Kennedy Press Site will be open for shuttle Atlantis’ rollout to Launch Pad 39A scheduled for 8 p.m. Tuesday and will remain open until 4:30 p.m. Wednesday.News media representatives who have been approved for STS-134 mission badges but have not picked them up yet may do so at NASA's Pass and Identification Building on State Road 3 on May 31 from 4 - 6 p.m. and 10:30 p.m. to 12:30 a.m. on June 1.The last bus will depart from the news center for the Shuttle Landing Facility one hour before landing.If the shuttle landing is diverted to Edwards after Wednesday, reporters should call the public affairs office at NASA's Dryden Flight Research Center at 661-276-3449. Dryden has limited facilities available for previously accredited journalists.

Spitzer Sees Crystal Rain in Infant Star Outer Clouds

Tiny crystals of a green mineral called olivine are falling down like rain on a burgeoning star, according to observations from NASA's Spitzer Space Telescope. This is the first time such crystals have been observed in the dusty clouds of gas that collapse around forming stars. Astronomers are still debating how the crystals got there, but the most likely culprits are jets of gas blasting away from the embryonic star.

You need temperatures as hot as lava to make these crystals, said Tom Megeath of the University of Toledo in Ohio. He is the principal investigator of the research and the second author of a new study appearing in Astrophysical Journal Letters. "We propose that the crystals were cooked up near the surface of the forming star, and then carried up into the surrounding cloud where temperatures are much colder, and ultimately fell down again like glitter."

Spitzer's infrared detectors spotted the crystal rain around a distant, sun-like embryonic star, or protostar, referred to as HOPS-68, in the constellation Orion. The Spitzer observations were made before it used up its liquid coolant in May 2009 and began its warm mission.

Endeavour's Late Inspection Complete

Space shuttle Endeavour's crew completed today's inspection of the shuttle's thermal protection system at 2:16 a.m. EDT. The crew began the inspection early. They used the 50-foot-long Orbiter Boom Sensor System to conduct a high fidelity, three-dimensional scan of areas of the shuttle that experience the highest heating during entry - the wing leading edges and nose cap. Managers and engineers in Mission Control will review the data to validate the heat shield's integrity and assure it has suffered no significant micrometeoroid and orbital debris damage.

The late inspection occurred earlier in the mission than normal, prior to undocking. As a consequence, the risk of re-entering with undetected micrometeoroid debris is increased but deemed acceptable.

During the mission's fourth and final spacewalk on Friday, the boom will be left at the space station to extend the robotic reach. Mike Fincke and Greg Chamitoff will prepare it for its stay by replacing its grapple fixture with a power data grapple fixture to enable its use as the new International Space Station Boom Assembly. Once on station without power and in the extended exposure to the vacuum of space, the boom's imagery sensors will cease functioning.

Asteroid Research Begins Under the Sea

NASA is using a capability-driven approach to new concepts of human exploration for multiple destinations in our solar system; one of those destinations are near-Earth asteroids. Across the agency, experts are being called into action to develop solutions to this new challenge. In particular, the NEEMO 15 analog field test, slated for mid-October this year, will test new tools, techniques, time lining approaches and communication technologies which could be useful when humans approach asteroids in space.

During the week of May 9-15, 2011, the NEEMO 15 support team is conducting engineering evaluations in the Aquarius undersea research laboratory in Key Largo, Fla. The purpose of these engineering tests is to understand the equipment, techniques and test concepts that will be implemented in the October NEEMO 15 mission, to make sure that all systems are ready for more rigorous testing when the crew will be living full-time in the Aquarius undersea habitat.

The specific operations for visiting an asteroid have not been considered in great detail before. Gravity on an asteroid is negligible, so walking around on one isn't really an option. Anchoring to the surface will probably be necessary, but asteroids are made up of different materials - some solid metal, some piles of rubble and some, a combination of rock, pebbles and dust. Weak gravity and diverse materials present problems whose solutions can be experimented with on the ocean floor, which is what the NEEMO 15 mission is trying to do.

NEEMO 15 will focus on three different aspects of a mission to an asteroid surface. The first is anchoring to the surface of the asteroid. Unlike the moon or Mars, an asteroid would have little, if any, gravity to hold astronauts or vehicles to its surface, so an anchor would be necessary. To move around on the surface of an asteroid will require a method of connecting multiple anchors to form pathways. The best way in which to connect these anchors will be the second aspect of a near-Earth asteroid mission addressed by NEEMO 15. Finally, since NASA's purpose in visiting an asteroid would be for scientific research, the third aspect of this mission investigated by NEEMO 15 would be different methods of sample collection.

NASA's Next Mars Rover Nears Completion

Assembly and testing of NASA's Mars Science Laboratory spacecraft is far enough along that the mission's rover, Curiosity, looks very much as it will when it is investigating Mars.

Testing continues this month at NASA's Jet Propulsion Laboratory, Pasadena, Calif., on the rover and other components of the spacecraft that will deliver Curiosity to Mars. In May and June, the spacecraft will be shipped to NASA Kennedy Space Center, Fla., where preparations will continue for launch in the period between Nov. 25 and Dec. 18, 2011.

The mission will use Curiosity to study one of the most intriguing places on Mars -- still to be selected from among four finalist landing-site candidates. It will study whether a selected area of Mars has offered environmental conditions favorable for microbial life and for preserving evidence about whether Martian life has existed.

China's First Space Station: A New Foothold in Earth Orbit

China's state-run news outlets report that preparations of the country's first space station module, called Tiangong-1, are in full swing for a launch in the second half of this year and will be followed by an unpiloted spacecraft.

The spacecraft twosome, the station module and China's Shenzhou 8 vehicle, will mark the country's first round of orbital rendezvous and docking tests – viewed as a springboard to larger space adventures. A Long March 2F rocket is the booster of choice for the individual launches, according to reports by China's Xinhua news agency.

According to state media reports, the Tiangong-1 space station module is outfitted with a docking port on its front and rear ends. It will tip the scales at roughly 8 1/2 tons and purportedly will have a two-year lifetime in Earth orbit. Next year, China's Shenzhou 9 and Shenzhou 10 missions, each carrying astronauts, are expected to link up with the station module, according to current plan.

read more

Largest 3-D Map Opens Window to the Ancient Universe

The largest-ever three-dimensional map of the distant universe has been created using the light of the brightest objects in the cosmos. Since this distant light took eons to reach Earth, the map is essentially a window back in time, providing an unprecedented view of what the universe looked like 11 billion years ago.Normally, researchers make maps of the universe by looking at galaxies.

"Here, we are looking at intergalactic hydrogen gas, which blocks light," said researcher Anže Slosar, a physicist at the U.S. Department of Energy's Brookhaven National Laboratory. "It's like looking at the moon through clouds -- you can see the shapes of the clouds by the moonlight that they block."

read more

A Galactic Rose Highlights Hubble's 21st Anniversary

In celebration of the 21st anniversary of the Hubble Space Telescope's deployment into space, astronomers pointed Hubble at an especially photogenic group of interacting galaxies called Arp 273.

This image, taken by the NASA/ESA Hubble Space Telescope, shows a group of interacting galaxies called Arp 273. The larger of the spiral galaxies, known as UGC 1810, has a disc that is tidally distorted into a rose-like shape by the gravitational pull of the companion galaxy below it, known as UGC 1813. The swathe of blue jewels across the top is the combined light from clusters of intensely bright and hot young blue stars. These massive stars glow fiercely in ultraviolet light.

The smaller, nearly edge-on companion shows distinct signs of intense star formation at its nucleus, perhaps triggered by the encounter with the companion galaxy.

Russian Spaceship 'Gagarin' Arrives at Space Station

A Russian spaceship bearing the name of history's most famous cosmonaut docked at the International Space Station late Wednesday to deliver three new crew members to the orbiting lab. The Soyuz TMA-21 — nicknamed "Gagarin" after Yuri Gagarin, who became the first person in space on April 12, 1961 — successfully docked with the station's Poisk module at 7:09 p.m. EDT (2309 GMT). The spacecraft had launched from Baikonur Cosmodrome in Kazakhstan on April 4, blasting off from the same pad used for Gagarin's historic flight nearly 50 years ago. "Contact and capture — docking confirmed," a NASA official announced as the "Gagarin" sidled up to the orbiting lab. The "Gagarin" launched into space Monday (April 4 EDT) carrying two cosmonauts and one NASA astronaut to join three other crewmembers already aboard the station, rounding out the orbiting lab's Expedition 27.

The three spaceflyers — NASA's Ron Garan and Russians Alexander Samokutyaev and Andrey Borisenko — will also stay on as part of the next station mission, Expedition 28. "It was a great couple of days and we're ready to get to work," Garan said. Garan and Samokutyaev will be flight engineers on both expeditions. Borisenko will serve as a flight engineer on Expedition 27 and later serve as the commander of Expedition 28. [Vote Now! The Best Spaceships of All Time]. The crew received a flood of congratulatory calls from Russia's Mission Control center near Moscow after docking at the space station. Russian space official and the families of the astronaut and cosmonauts were on hand to wish the crew well. "We love you," Garan's wife Carmel told her husband and his crewmates after their arrival on the station. "We'll keep the fires burning at home, and we'll welcome you home with open arms at the end of your successful mission."

NASA astronaut launch video

NASA astronaut Scott Kelly and Russian cosmonauts Oleg Skripochka and Alexander Kaleri launched in their Soyuz TMA-01M spacecraft from the Baikonur Cosmodrome in Kazakhstan Thursday at 7:10 p.m. EDT (Friday, Kazakhstan time) beginning a two-day journey to the International Space Station.

Less than 10 minutes after launch, their spacecraft reached orbit and its antennas and solar arrays were deployed.

The trio will dock to the Poisk module Saturday at 8:02 p.m. completing the Expedition 25 crew. Kelly, Skripochka and Kaleri will begin a five-month tour of duty aboard the orbiting laboratory.

Welcoming them aboard will be current station residents, Expedition 25 Commander Doug Wheelock and Flight Engineers Fyodor Yurchikhin and Shannon Walker. Wheelock, Yurchikhin and Walker arrived June 17 aboard their Soyuz TMA-19 spacecraft.

MAVEN Mission to Investigate How Sun Steals Martian Atmosphere

The Red Planet bleeds. Not blood, but its atmosphere, slowly trickling away to space. The culprit is our sun, which is using its own breath, the solar wind, and its radiation to rob Mars of its air. The crime may have condemned the planet's surface, once apparently promising for life, to a cold and sterile existence.

Features on Mars resembling dry riverbeds, and the discovery of minerals that form in the presence of water, indicate that Mars once had a thicker atmosphere and was warm enough for liquid water to flow on the surface. However, somehow that thick atmosphere got lost in space. It appears Mars has been cold and dry for billions of years, with an atmosphere so thin, any liquid water on the surface quickly boils away while the sun's ultraviolet radiation scours the ground.

Two Asteroids to Pass by Earth

Two asteroids, several meters in diameter and in unrelated orbits, will pass within the moon's distance of Earth on Wednesday, Sept. 8.

Both asteroids should be observable near closest approach to Earth with moderate-sized amateur telescopes. Neither of these objects has a chance of hitting Earth. A 10-meter-sized near-Earth asteroid from the undiscovered population of about 50 million would be expected to pass almost daily within a lunar distance, and one might strike Earth's atmosphere about every 10 years on average.

The Catalina Sky Survey near Tucson, Ariz., discovered both objects on the morning of Sunday, Sept. 5, during a routine monitoring of the skies. The Minor Planet Center in Cambridge, Mass., first received the observations Sunday morning, determined preliminary orbits and concluded that both objects would pass within the distance of the moon about three days after their discovery.

Near-Earth asteroid 2010 RX30 is estimated to be 32 to 65 feet (10 to 20 meters) in size and will pass within 0.6 lunar distances of Earth (about 154,000 miles, or 248,000 kilometers) at 2:51 a.m. PDT (5:51 a.m. EDT) Wednesday. The second object, 2010 RF12, estimated to be 20 to 46 feet (6 to 14 meters) in size, will pass within 0.2 lunar distances (about 49,088 miles or 79,000 kilometers) a few hours later at 2:12 p.m. PDT (5:12 pm EDT).

Crew Readies for Resupply Ship and Upcoming Departure

The Expedition 24 crew members are preparing for the arrival of the ISS Progress 39 cargo craft to replenish the orbiting laboratory with food, fuel, supplies and other cargo. The Progress 39 will dock to the aft end of the Zvezda service module Friday, Sept. 10. It is replacing the trash-filled Progress 38 which undocked Aug. 31 and is poised to re-enter Earth’s atmosphere Monday for a fiery destruction over the Pacific Ocean.

The crew also will have an off-duty day Monday due to a frenetic pace of science activities. The six crew members are relaxing after three repair spacewalks restored the station’s cooling system.

Hurricane activity captured the attention of the station residents as they photographed and videotaped Earl churning in the Atlantic Ocean. The imagery and video are downlinked to ground controllers for observation and study by scientists. A Russian experiment, Uragan (Hurricane), monitors and studies the catastrophic effects of natural and man-made disasters. Other ongoing Earth observation experiments aboard the orbiting laboratory study natural phenomena and human activities and their consequences on the planet.