• 2010 nasa special
    a total eclipse of the Sun is visible from within a narrow corridor that traverses Earth's southern Hemisphere. The path of the Moon's umbral shadow crosses the South Pacific Ocean where it makes no landfall except for Mangaia (Cook Islands) and Easter Island (Isla de Pascua).
Showing posts with label NASA Space Information. Show all posts
Showing posts with label NASA Space Information. Show all posts

NASA Aerospace Safety Advisory Panel Meeting

Event Format: Advisory Meeting

Date: Tuesday, May 24, 2011

Location: NASA Headquarters, Room 9H40, 300 E. Street, SW., Washington DC, DC 20546, US

[Federal Register Volume 76, Number 88 (Friday, May 6, 2011)] [Notices] [Pages 26316-26317] From the Federal Register Online via the Government Printing Office [www.gpo.gov] [FR Doc No: 2011-11028]
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION 

[Notice 11- 044]
Aerospace Safety Advisory Panel Meeting
ACTION: Notice of meeting; Correction. 

Federal Register Citation of Previous Announcement: 76 FR 23339, Notice Number 11-043, dated April 26, 2011; and 76 FR 19147, Notice Number 11-030, dated April 6, 2011.
SUMMARY: The National Aeronautics and Space Administration published a notice in the Federal Register of April 26, 2011, announcing a meeting of the Aerospace Safety Advisory Panel (ASAP) to take place on May 24, 2011, at the Kennedy Space Center, FL. 

Correction: Date and time of ASAP public meeting remains the same: Tuesday, May 24, 2011, 11 a.m. to 1 p.m. Location has been moved to: NASA Headquarters, Room 9H40, 300 E. Street, SW., Washington, DC 20546. Agenda has been modified accordingly. 

FOR FURTHER INFORMATION CONTACT: Ms. Kathy Dakon, ASAP Executive Director, National Aeronautics and Space Administration, Washington, DC 20546, (202) 358-0732. 

SUPPLEMENTARY INFORMATION: The Aerospace Safety Advisory Panel will hold its 2nd Quarterly Meeting for 2011. This discussion is pursuant to carrying out its statutory duties for which the Panel reviews, identifies, evaluates, and advises on those program activities, systems, procedures, and management activities that can contribute to program risk. Priority is given to those programs that involve the safety of human flight.

The agenda will include: Updates on Safety and Mission Assurance; Safety Metrics; and Commercial Space

The meeting will be open to the public up to the seating capacity of the room. Seating will be on a first-come basis. Photographs will only be permitted during the first 10 minutes of the meeting. During the first 30 minutes of the meeting, members of the public may make a 5-minute verbal presentation to the Panel on the subject of safety in NASA. To do so, please contact Ms. Susan Burch at susan.burch@nasa.gov or by telephone at (202) 358-0550 at least 48 hours in advance. Any member of the public is permitted to file a written statement with the Panel at the time of the meeting. 

Verbal presentations and written comments should be limited to the subject of safety in NASA. Attendees will be requested to sign a register and to comply with NASA security requirements, including the presentation of a valid picture ID, before receiving an access badge. 

Foreign nationals attending this meeting will be required to provide a copy of their passport, visa, or green card in addition to providing the following information no less than 10 working days prior to the meeting: Full name; gender; date/place of birth; citizenship; visa/green card information (number, type, expiration date); 

passport information (number, country, expiration date); employer/affiliation information (name of institution, address, country, telephone); title/position of attendee. To expedite admittance, attendees with U.S. citizenship can provide identifying information 3 working days in advance by contacting Susan Burch via e-mail at susan.burch@nasa.gov or by telephone at (202) 358-0550. 

It is imperative that the meeting be held on this date to accommodate the scheduling priorities of the key participants. 

May 2, 2011. P. Diane Rausch, Advisory Committee Management Officer, National Aeronautics and Space Administration. [FR Doc. 2011-11028 Filed 5-5-11; 8:45 am] BILLING CODE P

Exploring the Wonders of the Universe

Exploring the Wonders of the Universe

The newly-installed Alpha Magnetic Spectrometer-2 is visible at center of the International Space Station's starboard truss. The Alpha Magnetic Spectrometer, or AMS, is the largest scientific collaboration to use the orbital laboratory. 

This investigation is sponsored by the U.S. Department of Energy and made possible by funding from 16 nations. Led by Nobel Laureate Samuel Ting, more than 600 physicists from around the globe will be able to participate in the data generated from this particle physics detector. 

The mission of the AMS is, in part, to seek answers to the mysteries of antimatter, dark matter and cosmic ray propagation in the universe. 

 International Space Station

 

Since 1981, NASA space shuttles have been rocketing from the Florida coast into Earth orbit. The five orbiters — Columbia, Challenger, Discovery, Atlantis and Endeavour — have flown more than 130 times, carrying over 350 people into space and travelling more than half a billion miles, more than enough to reach Jupiter. Designed to return to Earth and land like a giant glider, the shuttle was the world's first reusable space vehicle. More than all of that, though, the shuttle program expanded the limits of human achievement and broadened our understanding of our world.

It all started with STS-1, launched on April 12, 1981, just twenty years to the day after Soviet cosmonaut Yuri Gagarin became the first human in space. When astronauts John Young and Robert Crippen launched that morning in Columbia, it was the first time in history a new spacecraft was launched on its maiden voyage with a crew aboard.
For an entire generation, the space shuttle was NASA. We've watched a parade of firsts -- Sally Ride, Guy Bluford, Kathy Sullivan, John Glenn and others. We've seen astronauts float free, and launch and repair spacecraft like Hubble which have fundamentally changed our understanding of the universe.

In this feature, we look back at the Shuttle's historic missions, the people it flew into space, and its achievements.

Space Shuttle Mission: STS-134

Commander Mark Kelly and Mission Specialist Mike Fincke 

Image above: Commander Mark Kelly (left) and Mission Specialist Mike Fincke aboard space shuttle Endeavour talk to students at Mesa Verde Elementary School in Tucson, Ariz. Photo credit: NASA TV

The crew members for space shuttle Endeavour's STS-134 mission are Commander Mark Kelly, Pilot Gregory H. Johnson and Mission Specialists Michael Fincke, Greg Chamitoff, Andrew Feustel and European Space Agency astronaut Roberto Vittori.

During the 16-day mission, Endeavour and its crew will deliver the Alpha Magnetic Spectrometer (AMS) and spare parts including two S-band communications antennas, a high-pressure gas tank and additional spare parts for Dextre.

The Power of A Moon Rock

"This is a moon rock and it's on our kitchen table. This rock encapsulates all of the optimism and unlimited potential that Americans had at the time. It made me believe that anything is possible. I wanted kids of this generation to have this experience. So, although it wasn't easy -- I borrowed a Moon Rock from NASA."
--Debra Sea in "Moon Rock"
Between 1969 and 1972 six Apollo missions brought back 382 kilograms (842 pounds) of lunar rocks, core samples, pebbles, sand and dust from the lunar surface. The six space flights returned 2,200 separate samples from six different exploration sites on the Moon.

Debra Sea and her brothers, David and William, admire an Apollo 11 moon rock on their kitchen table

In 1970, Debra Sea and her brothers, David and William, admire a Moon Rock from Apollo 11 as it sits atop their kitchen table.

Credit: Sea Family
To view the film, "Moon Rock," by Debra Sea, please visit:

moonrockthemovie.com/movie.html
The sample that sat before Debra and two of her younger brothers in 1970 returned to Earth from Apollo 11. And it landed on her kitchen table by way of her father, Duane Sea, a former a NASA science demonstrator, also known as a Spacemobiler.

Duane and his Spacemobile traveled to schools across the Mid-West, reaching more than 400,000 students. In the summer, Debra and her siblings would go along for the ride.

"Like everyone else, we were wildly optimistic about the future of space science," Debra said.

At age 10, her Moon Rock experience was documented with a photograph, which was labeled as "Moon Rock" in her family album. So, it was only natural that her film would also be labeled as "Moon Rock."

"It was always a story I wanted to tell," said Debra. "The timing was perfect."

Perfect because she was a working on her Master's of Fine Arts (MFA) at the University of North Carolina Greensboro when she chose "Moon Rock" as her Master Production film project. She was one of three students chosen to receive a 2011 Carole Fielding Student Grants awarded by the University Film and Video Association.

Debra Sea with Apollo 14 moon rock 

For her thesis film, "Moon Rock," Debra Sea borrowed a Moon Rock from NASA's Langley Research Center in Hampton, Va.

Credit: NASA/Sean Smith
But Debra quickly learned that borrowing a Moon Rock from NASA was no easy task.

After six months and a great deal of determination, her Lunar Sample Application was approved. For pick-up, she was referred to NASA's Langley Research Center in Hampton, Va., because it was in her outreach region.

The larger, display Moon Rocks are considered a national treasure that cannot be shipped, only hand carried. With possession, comes a strict set of guidelines. It must be kept in sight or in a safe. It can't be kept in a motel room overnight. And don't touch the Lucite without gloves, because the oil from skin can damage and cloud the Lucite.

"We were like old friends," Debra said of the Moon Rock. Except this was a different rock -- from Apollo 14. And this time, she was responsible for it. That was quite the burden for Debra, who constantly worried about the rock, much like a mother worries for her child.

Meghan Guethe, Langley's exhibits manager, helped Debra through the process. She understood and appreciated Debra's desire to keep it safe. "Everything is priced when it is sent out with an exhibit," Guethe said. "We cannot price these."

Debra Sea and her brothers beside their father's Spacemobile van 

In the summer, Debra Sea and her brothers would travel in a Spacemobile driven by their father Duane, a former NASA Science demonstrator, also known as a Spacemobiler.

Credit: Sea Family
It took a lot of planning to prepare the invaluable Moon Rock's trip to three classrooms at Wadena-Deer Creek, a K-12 school in Minnesota, where Debra's brother David teaches. She created a contingency plan for each airport.

And when she and her film assistant Adrienne Ostberg, a first-year MFA student, had their last flight canceled, they rotated staying with the rock in a private, locked room, purposed for nursing moms.

Their "baby" was a Moon Rock, which was enclosed in a Lucite pyramid. The 115-gram rock had its own carrying case and a small brass plate on the case reads, "IF FOUND, RETURN TO -- NASA, JOHNSON SPACE CENTER, HOUSTON, TEXAS 77058."

Duane accompanied her to the school. And despite the fact that he hadn't worked for NASA in 40 years, he smoothly converted back into his Spacemobiler ways.

"Have you ever driven a nail with a banana?" Duane asked the students after dipping one into a container of liquid nitrogen and freezing it solid.

As the banana proved to have the power of a hammer, the looks of authentic amazement and surprise on the student's faces spoke powerfully. And so did their questions.

Apollo 14 moon rock 
This Moon Rock, from Apollo 14, visited three classes at Wadena-Deer Creek, a K-12 school in Minnesota, where Debra's brother David teaches.
Credit: NASA/Sean Smith
"Is this a magic trick?" a student asked.

"No, magic. Just science" Duane replied.

"He had such a presence," Debra said of her father.

The Moon Rock temporarily abolished his presence. The students put gloves on and one-by-one touched the pyramid and gazed into the rock that had traveled some 238,857 miles (384,403 km) back to Earth 40 years prior.

"Everyone wanted to touch it, like a relic," Debra said of the students, and even airport security personnel that help her to guard it from harm.

But the contact that truly mattered was that of the students.

"I keep hearing that kids are different today than they were years ago. I just don't buy that," Duane said. "Kids are kids. The same eager faces that you see in front of you today are the same that I saw in front of me 40 years ago."

Debra and two of her brothers recreated the "Moon Rock" photo, and the moment that sparked their own sense of wonder. It seemingly had a great affect on them as each studied and works in a science-related field.

Whether Science or magic, their Moon Rock experience was afforded to a new generation. And now, it's up to them to decide what to do with it.

"I see incredible optimism and potential in these kids. And after bringing the Moon Rock home, I feel really hopeful about the future," Debra said. "I still believe that anything is possible. And I know I always will."

 
 
Denise Linberry
The Researcher News
NASA Langley Research Center

Update 3: NASA captures satellite images of 2011 Mississippi floods

NASA unveiled  a series of satellite images of the current Mississippi flooding on May 18 showing the major flooding of the Mississippi River around Memphis, and other states . NASA's fleet of Earth-observing satellites have been gathering data on the current Mississippi flooding as well as floods worldwide.

On May 18, 2011, the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Terra satellite observed water in the Morganza Floodway along the Mississippi River.

The Mississippi River reached nearly 48 feet in Memphis, Tenn., on May 10, according to the U.S. National Weather Service. It was the highest water level for Memphis since 1937.

This month muddy water has pushed over the Mississippi's banks both east and west of the normal river channel. Flood waters span the distance between Memphis and West Memphis.

MODIS acquired the top image on May 18, 2011, and the bottom image on May 4, 2011. Both images use a combination of visible and infrared light to increase contrast between water and land. Water ranges in color from gray-blue to navy. (Lake Pontchartrain appears silvery blue on May 18 due largely to the angle of sunlight.) Vegetation is green. Bare ground is brown. Clouds are pale blue-green and cast shadows.

Both images show flooded conditions along the Mississippi River. A significant difference between the images, however, is the water visible in the Morganza Floodway on May 18. The Army Corps of Engineers reported that the discharge in the floodway was 108,000 cubic feet per second on May 18, the floodway's fifth day of operation in 2011.


On May 18, 2011, the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite observed water in the Morganza Floodway along the Mississippi River. As the U.S. Army Corps of Engineers explains, the floodway is designed to ease water levels in downstream communities along the Mississippi by diverting some water into the Atchafalaya Basin.  MODIS acquired the top image on May 18, 2011, and the bottom image on May 4, 2011. Both images use a combination of visible and infrared light to increase contrast between water and land. Water ranges in color from gray-blue to navy. (Lake Pontchartrain appears silvery blue on May 18 due largely to the angle of sunlight.) Vegetation is green. Bare ground is brown. Clouds are pale blue-green and cast shadows.  Both images show flooded conditions along the Mississippi River. A significant difference between the images, however, is the water visible in the Morganza Floodway on May 18. The Army Corps of Engineers reported that the discharge in the floodway was 108,000 cubic feet per second on May 18, the floodway’s fifth day of operation in 2011.  The Advanced Hydrological Prediction Service (AHPS) of the U.S. National Weather Service reported that the Mississippi River at Baton Rouge reached 44.85 feet (13.67 meters) at 2:00 p.m. CDT on May 18. This level was below the city’s record flood level of 47.28 feet (14.41 meters) set in 1927. As of May 18, the Mississippi River was projected to remain at roughly the same level at Baton Rouge through May 23.
 
On May 18, 2011, the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite observed water in the Morganza Floodway along the Mississippi River. As the U.S. Army Corps of Engineers explains, the floodway is designed to ease water levels in downstream communities along the Mississippi by diverting some water into the Atchafalaya Basin. MODIS acquired the top image on May 18, 2011, and the bottom image on May 4, 2011. Both images use a combination of visible and infrared light to increase contrast between water and land. Water ranges in color from gray-blue to navy. (Lake Pontchartrain appears silvery blue on May 18 due largely to the angle of sunlight.) Vegetation is green. Bare ground is brown. Clouds are pale blue-green and cast shadows. Both images show flooded conditions along the Mississippi River. A significant difference between the images, however, is the water visible in the Morganza Floodway on May 18. The Army Corps of Engineers reported that the discharge in the floodway was 108,000 cubic feet per second on May 18, the floodway’s fifth day of operation in 2011. The Advanced Hydrological Prediction Service (AHPS) of the U.S. National Weather Service reported that the Mississippi River at Baton Rouge reached 44.85 feet (13.67 meters) at 2:00 p.m. CDT on May 18. This level was below the city’s record flood level of 47.28 feet (14.41 meters) set in 1927. As of May 18, the Mississippi River was projected to remain at roughly the same level at Baton Rouge through May 23.
 
On May 18, 2011, the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite observed water in the Morganza Floodway along the Mississippi River. As the U.S. Army Corps of Engineers explains, the floodway is designed to ease water levels in downstream communities along the Mississippi by diverting some water into the Atchafalaya Basin.  MODIS acquired the top image on May 18, 2011, and the bottom image on May 4, 2011. Both images use a combination of visible and infrared light to increase contrast between water and land. Water ranges in color from gray-blue to navy. (Lake Pontchartrain appears silvery blue on May 18 due largely to the angle of sunlight.) Vegetation is green. Bare ground is brown. Clouds are pale blue-green and cast shadows.  Both images show flooded conditions along the Mississippi River. A significant difference between the images, however, is the water visible in the Morganza Floodway on May 18. The Army Corps of Engineers reported that the discharge in the floodway was 108,000 cubic feet per second on May 18, the floodway’s fifth day of operation in 2011.  The Advanced Hydrological Prediction Service (AHPS) of the U.S. National Weather Service reported that the Mississippi River at Baton Rouge reached 44.85 feet (13.67 meters) at 2:00 p.m. CDT on May 18. This level was below the city’s record flood level of 47.28 feet (14.41 meters) set in 1927. As of May 18, the Mississippi River was projected to remain at roughly the same level at Baton Rouge through May 23.
 
On May 18, 2011, the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite observed water in the Morganza Floodway along the Mississippi River. As the U.S. Army Corps of Engineers explains, the floodway is designed to ease water levels in downstream communities along the Mississippi by diverting some water into the Atchafalaya Basin.
 
MODIS acquired the top image on May 18, 2011, and the bottom image on May 4, 2011. Both images use a combination of visible and infrared light to increase contrast between water and land. Water ranges in color from gray-blue to navy. (Lake Pontchartrain appears silvery blue on May 18 due largely to the angle of sunlight.) Vegetation is green. Bare ground is brown. Clouds are pale blue-green and cast shadows. Both images show flooded conditions along the Mississippi River. A significant difference between the images, however, is the water visible in the Morganza Floodway on May 18. 
 
The Army Corps of Engineers reported that the discharge in the floodway was 108,000 cubic feet per second on May 18, the floodway’s fifth day of operation in 2011. The Advanced Hydrological Prediction Service (AHPS) of the U.S. National Weather Service reported that the Mississippi River at Baton Rouge reached 44.85 feet (13.67 meters) at 2:00 p.m. CDT on May 18. This level was below the city’s record flood level of 47.28 feet (14.41 meters) set in 1927. As of May 18, the Mississippi River was projected to remain at roughly the same level at Baton Rouge through May 23.
 
Following are Images of Morganza,  Arkansas,  Tennesse,  from NASA:

On May 14, 2011, the U.S. Army Corps of Engineers opened the Morganza Spillway in an attempt to ease flooding along the Mississippi River in Louisiana. The decision was made to protect the heavily populated areas and infrastructure around the ports of Baton Rouge and New Orleans. The decision is not without cost, however, to the thousands of people who are likely to lose homes and farms within the flood plain downstream.  On May 15, the Advanced Land Imager (ALI) on NASA’s Earth Observing-1 (EO-1) satellite captured this natural-color image (top) of the Morganza Floodway. The image was acquired at 11:20 a.m. Central Daylight Time, one day after the spillway was partially opened. The lower photo was taken on May 14 by the Army Corps, several hours after water began streaming onto the floodway.  The flood control structure, or spillway, includes 125 gates, 11 of which had been opened as of noon on May 16. In the satellite image, the white pixels near the spillway are whitewater churned up by the flow through the gates; the downloadable large image shows this in much finer detail. Square and quadrilateral shapes on the landscape show areas that were cleared for farming or perhaps shaped for flood control earthworks.  In the natural color satellite, water ranges in colors of olive, tan, black, and gray, reflecting the different loads of muddy sediment churned up from the bottom; darker areas might also reflect deeper water. Past the spillway, water is more readily apparent along the levee on the south and east side of the floodway, suggesting that there are fewer trees and perhaps lower elevations in those areas. Potential inundation maps (PDF) from the Army Corps appear to confirm that, as water levels are projected to rise to 10–15 feet (3–4.5 meters) in the southern and eastern areas and 5–10 feet (1.5–3 meters) in the northern and western areas in the image above.  Green areas do not necessarily mean a lack of water. As the aerial photo shows, much of the floodway is covered with trees that will shield the water below from the eyes of satellite sensors. Water is somewhat easier to spot in the near-infrared and shortwave infrared image linked below the top photo.  Video of the opening of the Morganza Floodway can be viewed online here. The floodway was last opened in 1973, the first and only time it was used before 2011.
 
On May 14, 2011, the U.S. Army Corps of Engineers opened the Morganza Spillway in an attempt to ease flooding along the Mississippi River in Louisiana. The decision was made to protect the heavily populated areas and infrastructure around the ports of Baton Rouge and New Orleans. The decision is not without cost, however, to the thousands of people who are likely to lose homes and farms within the flood plain downstream. On May 15, the Advanced Land Imager (ALI) on NASA’s Earth Observing-1 (EO-1) satellite captured this natural-color image (top) of the Morganza Floodway. The image was acquired at 11:20 a.m. Central Daylight Time, one day after the spillway was partially opened. 
 
he lower photo was taken on May 14 by the Army Corps, several hours after water began streaming onto the floodway. The flood control structure, or spillway, includes 125 gates, 11 of which had been opened as of noon on May 16. In the satellite image, the white pixels near the spillway are whitewater churned up by the flow through the gates; the downloadable large image shows this in much finer detail. Square and quadrilateral shapes on the landscape show areas that were cleared for farming or perhaps shaped for flood control earthworks. I
 
n the natural color satellite, water ranges in colors of olive, tan, black, and gray, reflecting the different loads of muddy sediment churned up from the bottom; darker areas might also reflect deeper water. Past the spillway, water is more readily apparent along the levee on the south and east side of the floodway, suggesting that there are fewer trees and perhaps lower elevations in those areas. Potential inundation maps (PDF) from the Army Corps appear to confirm that, as water levels are projected to rise to 10–15 feet (3–4.5 meters) in the southern and eastern areas and 5–10 feet (1.5–3 meters) in the northern and western areas in the image above. 
 
Green areas do not necessarily mean a lack of water. As the aerial photo shows, much of the floodway is covered with trees that will shield the water below from the eyes of satellite sensors. Water is somewhat easier to spot in the near-infrared and shortwave infrared image linked below the top photo. Video of the opening of the Morganza Floodway can be viewed online here. The floodway was last opened in 1973, the first and only time it was used before 2011.
 
The Mississippi River spilled over its banks in Arkansas and Tennessee on May 12, 2011, as the International Space Station passed overhead. This astronaut photograph shows muddy water sitting on floodplains around Tomato, Arkansas, as well as extensive flooding to the north.  Flood waters around Tomato appear confined by an embankment in the west. The embankment extends southward from a bend in the Mississippi. West of the embankment lies a patchwork of agricultural fields. East of the river lies an expanse of dark green forest, the Anderson-Tully State Wildlife Management Area.
 
The Mississippi River spilled over its banks in Arkansas and Tennessee on May 12, 2011, as the International Space Station passed overhead. This astronaut photograph shows muddy water sitting on floodplains around Tomato, Arkansas, as well as extensive flooding to the north. Flood waters around Tomato appear confined by an embankment in the west. The embankment extends southward from a bend in the Mississippi. West of the embankment lies a patchwork of agricultural fields. East of the river lies an expanse of dark green forest, the Anderson-Tully State Wildlife Management Area.
 
Along a northward loop of the Mississippi River, near the city of New Madrid, flood water rested on agricultural fields in early May 2011. Taken from an altitude of 220 miles (350 kilometers) above the Earth, this astronaut photo shows muddy water filling a broad swath of cropland north of the river bend. In this image, north is toward the lower right.  Crops normally carpet the landscape north of New Madrid. This portion of Missouri, however, lies near the Birds Point-New Madrid Floodway. On May 2, 2011, the U.S. Army Corps of Engineers breached a levee near the confluence of the Ohio and Mississippi Rivers. The move spared the residents of Cairo, Illinois, but filled the floodway.
 
Along a northward loop of the Mississippi River, near the city of New Madrid, flood water rested on agricultural fields in early May 2011. Taken from an altitude of 220 miles (350 kilometers) above the Earth, this astronaut photo shows muddy water filling a broad swath of cropland north of the river bend. In this image, north is toward the lower right. Crops normally carpet the landscape north of New Madrid. This portion of Missouri, however, lies near the Birds Point-New Madrid Floodway. On May 2, 2011, the U.S. Army Corps of Engineers breached a levee near the confluence of the Ohio and Mississippi Rivers. The move spared the residents of Cairo, Illinois, but filled the floodway.
 
On May 13, 2011, the Mississippi River was approaching a record level at the city of Vicksburg, Mississippi, and had exceeded the previous record at Natchez, Miss. The Advanced Hydrological Prediction Service (AHPS) reported that the river reached 55.45 feet (16.90 meters) at 3:00 p.m. Central Daylight Time at Vicksburg, and 59.87 feet (18.25 meters) at 2:00 p.m. CDT at Natchez. The previous record for Natchez, set in 1937, was 58.04 feet (17.69 meters). The AHPS forecast that water levels would continue to rise in both locations.  The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA’s Terra satellite captured these false-color images of the area around Natchez on May 11, 2011 (top), and April 21, 2007 (bottom).  The images combine infrared, red, and green wavelengths to form a false-color image that distinguishes between muddy water and land. Water is blue, and sediment-laden water is a dull blue-green. Vegetation is red, and the brighter the red, the more robust the vegetation. Red and gray patches west of the river (top edge of each image) are agricultural fields. Clouds are white, and cast shadows onto the land surface below.  In May 2011, the Mississippi River pushed over its banks onto floodplains. In some places, the flood waters almost reached oxbow lakes along the river.
 
On May 13, 2011, the Mississippi River was approaching a record level at the city of Vicksburg, Mississippi, and had exceeded the previous record at Natchez, Miss. The Advanced Hydrological Prediction Service (AHPS) reported that the river reached 55.45 feet (16.90 meters) at 3:00 p.m. 
 
Central Daylight Time at Vicksburg, and 59.87 feet (18.25 meters) at 2:00 p.m. CDT at Natchez. The previous record for Natchez, set in 1937, was 58.04 feet (17.69 meters). The AHPS forecast that water levels would continue to rise in both locations. The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA’s Terra satellite captured these false-color images of the area around Natchez on May 11, 2011 (top), and April 21, 2007 (bottom). 
 
The images combine infrared, red, and green wavelengths to form a false-color image that distinguishes between muddy water and land. Water is blue, and sediment-laden water is a dull blue-green. Vegetation is red, and the brighter the red, the more robust the vegetation. Red and gray patches west of the river (top edge of each image) are agricultural fields. Clouds are white, and cast shadows onto the land surface below. In May 2011, the Mississippi River pushed over its banks onto floodplains. In some places, the flood waters almost reached oxbow lakes along the river.
 
On May 13, 2011, the Mississippi River was approaching a record level at the city of Vicksburg, Mississippi, and had exceeded the previous record at Natchez, Miss. The Advanced Hydrological Prediction Service (AHPS) reported that the river reached 55.45 feet (16.90 meters) at 3:00 p.m. Central Daylight Time at Vicksburg, and 59.87 feet (18.25 meters) at 2:00 p.m. CDT at Natchez. The previous record for Natchez, set in 1937, was 58.04 feet (17.69 meters). The AHPS forecast that water levels would continue to rise in both locations.  The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA’s Terra satellite captured these false-color images of the area around Natchez on May 11, 2011 (top), and April 21, 2007 (bottom).  The images combine infrared, red, and green wavelengths to form a false-color image that distinguishes between muddy water and land. Water is blue, and sediment-laden water is a dull blue-green. Vegetation is red, and the brighter the red, the more robust the vegetation. Red and gray patches west of the river (top edge of each image) are agricultural fields. Clouds are white, and cast shadows onto the land surface below.  In May 2011, the Mississippi River pushed over its banks onto floodplains. In some places, the flood waters almost reached oxbow lakes along the river.
 
On May 13, 2011, the Mississippi River was approaching a record level at the city of Vicksburg, Mississippi, and had exceeded the previous record at Natchez, Miss. The Advanced Hydrological Prediction Service (AHPS) reported that the river reached 55.45 feet (16.90 meters) at 3:00 p.m. Central Daylight Time at Vicksburg, and 59.87 feet (18.25 meters) at 2:00 p.m. CDT at Natchez. 
 
The previous record for Natchez, set in 1937, was 58.04 feet (17.69 meters). The AHPS forecast that water levels would continue to rise in both locations. 
 
The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA’s Terra satellite captured these false-color images of the area around Natchez on May 11, 2011 (top), and April 21, 2007 (bottom). The images combine infrared, red, and green wavelengths to form a false-color image that distinguishes between muddy water and land. Water is blue, and sediment-laden water is a dull blue-green. Vegetation is red, and the brighter the red, the more robust the vegetation. Red and gray patches west of the river (top edge of each image) are agricultural fields. Clouds are white, and cast shadows onto the land surface below. In May 2011, the Mississippi River pushed over its banks onto floodplains. In some places, the flood waters almost reached oxbow lakes along the river.
 
Following are Previous Images from NASA:

(Up) Landsat 5 shows the Mississippi River along the state borders of Tennessee, Kentucky, Missouri, and Arkansas on May 12, 2006. (bottom) Landsat 5 image shows the Mississippi River along the state borders of Tennessee, Kentucky, Missouri, and Arkansas on May 10, 2011. Credit: USGS/NASA //Remotely sensed data are not the only science endeavors occurring due to floods. The USGS collects river data through its network of about 7,700 stream gauges around the Nation. You can receive instant, customized updates about water conditions, including flooding, by subscribing to USGS WaterAlert. The scenes captured by Landsat 5 show the Mississippi River in the Memphis, Tenn. area, and along the state borders of Tennessee, Kentucky, Missouri, and Arkansas. The May 2006 images show the river before it began to flood. In the May images, the dark blue tones are water, the light green is cleared fields, and the light tones are clouds.
 
(Up) Landsat 5 shows the Mississippi River along the state borders of Tennessee, Kentucky, Missouri, and Arkansas on May 12, 2006. (bottom) Landsat 5 image shows the Mississippi River along the state borders of Tennessee, Kentucky, Missouri, and Arkansas on May 10, 2011. Credit: USGS/NASA //Remotely sensed data are not the only science endeavors occurring due to floods. 
 
The USGS collects river data through its network of about 7,700 stream gauges around the Nation. You can receive instant, customized updates about water conditions, including flooding, by subscribing to USGS WaterAlert. The scenes captured by Landsat 5 show the Mississippi River in the Memphis, Tenn. area, and along the state borders of Tennessee, Kentucky, Missouri, and Arkansas. The May 2006 images show the river before it began to flood. In the May images, the dark blue tones are water, the light green is cleared fields, and the light tones are clouds.
 
(Up) Landsat 5 shows the Mississippi River along the state borders of Tennessee, Kentucky, Missouri, and Arkansas on May 12, 2006. (bottom) Landsat 5 image shows the Mississippi River along the state borders of Tennessee, Kentucky, Missouri, and Arkansas on May 10, 2011. Credit: USGS/NASA //Remotely sensed data are not the only science endeavors occurring due to floods. The USGS collects river data through its network of about 7,700 stream gauges around the Nation. You can receive instant, customized updates about water conditions, including flooding, by subscribing to USGS WaterAlert. The scenes captured by Landsat 5 show the Mississippi River in the Memphis, Tenn. area, and along the state borders of Tennessee, Kentucky, Missouri, and Arkansas. The May 2006 images show the river before it began to flood. In the May images, the dark blue tones are water, the light green is cleared fields, and the light tones are clouds.
 
(Up) Landsat 5 shows the Mississippi River along the state borders of Tennessee, Kentucky, Missouri, and Arkansas on May 12, 2006. (bottom) Landsat 5 image shows the Mississippi River along the state borders of Tennessee, Kentucky, Missouri, and Arkansas on May 10, 2011. Credit: USGS/NASA //Remotely sensed data are not the only science endeavors occurring due to floods. The USGS collects river data through its network of about 7,700 stream gauges around the Nation. 
 
You can receive instant, customized updates about water conditions, including flooding, by subscribing to USGS WaterAlert. The scenes captured by Landsat 5 show the Mississippi River in the Memphis, Tenn. area, and along the state borders of Tennessee, Kentucky, Missouri, and Arkansas. The May 2006 images show the river before it began to flood. In the May images, the dark blue tones are water, the light green is cleared fields, and the light tones are clouds.
 
(Up) Landsat 5 image of the Mississippi River in the Memphis, Tenn. area on May 12, 2006. (bottom) Landsat 5 image of the Mississippi River in the Memphis, Tenn. area on May 10, 2011. Credit: USGS/NASA
 
(Up) Landsat 5 image of the Mississippi River in the Memphis, Tenn. area on May 12, 2006. (bottom) Landsat 5 image of the Mississippi River in the Memphis, Tenn. area on May 10, 2011. Credit: USGS/NASA
 
(UP) Landsat 5 image of the Mississippi River in the Memphis, Tenn. area on May 12, 2006. (bottom) Landsat 5 image of the Mississippi River in the Memphis, Tenn. area on May 10, 2011. Credit: USGS/NASA
 
(UP) Landsat 5 image of the Mississippi River in the Memphis, Tenn. area on May 12, 2006. (bottom) Landsat 5 image of the Mississippi River in the Memphis, Tenn. area on May 10, 2011. Credit: USGS/NASA
 
ISS027-E-027019 (12 May 2011) --- Parts of two states highly impacted by recent flooding of the Mississippi River, are pictured in this International Space Station image featuring an area east of Blytheville, Ark., off the right side of the image. Center point coordinates are located at 35.8 degrees north latitude and 89.7 degrees west longitude The areas of Ruckers Place, Tenn. and Tomato, Ark. are surrounded by water, while Barfield, Ark. is still dry behind the levee on the right side of the image. North is toward the bottom of the photo.
 
ISS027-E-027019 (12 May 2011) --- Parts of two states highly impacted by recent flooding of the Mississippi River, are pictured in this International Space Station image featuring an area east of Blytheville, Ark., off the right side of the image. Center point coordinates are located at 35.8 degrees north latitude and 89.7 degrees west longitude The areas of Ruckers Place, Tenn. and Tomato, Ark. are surrounded by water, while Barfield, Ark. is still dry behind the levee on the right side of the image. North is toward the bottom of the photo.
 
 ISS027-E-027019 (12 May 2011) --- Parts of two states highly impacted by recent flooding of the Mississippi River, are pictured in this International Space Station image featuring an area east of Blytheville, Ark., off the right side of the image. Center point coordinates are located at 35.8 degrees north latitude and 89.7 degrees west longitude The areas of Ruckers Place, Tenn. and Tomato, Ark. are surrounded by water, while Barfield, Ark. is still dry behind the levee on the right side of the image. North is toward the bottom of the photo.

ISS027-E-027023 (12 May 2011) --- An Expedition 27 crew member aboard the International Space Station, 220 miles above Earth and the Mississippi River, captured this May 12 still photo, clearly showing the outlines of some heavily flooded agricultural fields on the Missouri side of the river. The center point for this 400-mm frame is 36.27 degrees north latitude and 89.57 degrees west longitude (north of Caruthersville, Mo. and west of Ridgely, Tenn.). North is towards the lower right corner of the image.
 
ISS027-E-027023 (12 May 2011) --- An Expedition 27 crew member aboard the International Space Station, 220 miles above Earth and the Mississippi River, captured this May 12 still photo, clearly showing the outlines of some heavily flooded agricultural fields on the Missouri side of the river. The center point for this 400-mm frame is 36.27 degrees north latitude and 89.57 degrees west longitude (north of Caruthersville, Mo. and west of Ridgely, Tenn.). North is towards the lower right corner of the image.

Space Shuttle Mission: STS-134

The STS-134 crew members are welcomed aboard the station. 

Image above: Commander Mark Kelly and the STS-134 crew are welcomed aboard the International Space Station by the Expedition 27 crew. Photo credit: NASA TV

The crew members for space shuttle Endeavour's STS-134 mission are Commander Mark Kelly, Pilot Gregory H. Johnson and Mission Specialists Michael Fincke, Greg Chamitoff, Andrew Feustel and European Space Agency astronaut Roberto Vittori.

During the 16-day mission, Endeavour and its crew will deliver the Alpha Magnetic Spectrometer (AMS) and spare parts including two S-band communications antennas, a high-pressure gas tank and additional spare parts for Dextre.

Tornado Challenges Satellite Damage Track Detection Techniques

Satellite image of Alabama tornado damage 

A composite of two ASTER views over North Alabama taken May 5. The image extends from near the Tennessee border line to Jasper, Ala. Several tornado tracks are evident, including the Phil Campbell to Harvest track. These tracks are not as obvious as the Tuscaloosa tornado track. This is not because of a difference in intensity, but from the underlying surface over which the tornadoes occurred. (NASA) 
Satellite image of Alabama tornado damage 

High resolution ASTER image corresponds to the Google Earth image area of Northern Madison county region and the Harvest area. Tornado track is barely identifiable. (NASA)  

View annotated composite image
The Short-term Prediction Research and Transition, or SPoRT, team has used satellite data from the North Alabama region to identify tornado damage from the April 27th super storm outbreak.

NASA's Terra satellite, part of the Earth Observing System of satellites, captured images of the damage path. An instrument aboard Terra called the Advanced Spaceborne Thermal Emission and Reflection Radiometer, or ASTER, was used to discern vegetation contrasts over the region.

"This is the first time ASTER data has been applied to such a massive outbreak of storms," said Gary Jedlovec, atmospheric scientist at Marshall Space Flight Center. "The usefulness of satellite information in providing improved accuracy along with damage assessment in severe weather events continues to evolve."

The tornado track signature observed by ASTER is seen as a disruption in the vegetation or other reflective surfaces over a region caused by tornado winds. Uprooted trees quickly stop the process of photosynthesis and change color -- this is easily detected by satellite.

However, detecting damage in areas outside of heavy forestland is challenging.

In Madison and Limestone counties much of the area scarred by the tornadoes are agricultural in nature. Fields are either pasture land or row crops -- therefore the effect of tornado winds is minimal and the mark on satellite imagery is suppressed.

While this indicates a limitation to the use of this particular image analysis for tornado track detection over primarily agricultural land use, the SPoRT team is exploring the use of temperature channels from ASTER to better identify damage marks on Earth's surface. Terra/ASTER is a joint activity between NASA's Science Mission Directorate Earth Science Division and Japan's Ministry of Economy, Trade and Industry. Terra is one of 14 NASA satellites that look at the Earth to study and understand changes in the Earth system and provide societal benefits.

The NASA image created by the Short-term Prediction and Research Transition or SPoRT project at the Marshall Space Flight Center in Huntsville, using data provided courtesy of NASA Goddard Space Flight Center, the Land Processes Distributed Active Archive Center, Japan’s Earth Remote Sensing Data Analysis Center, the Ministry of Economy, Trade and Industry, along with the Japan Research Observation System Organization.
 
 


Janet Anderson, 256-544-0034
Marshall Space Flight Center, Huntsville, Ala.
Janet.L.Anderson@nasa.gov

The Far Side of the Moon -- And All the Way Around





image of lunar far side




Because the moon is tidally locked  And what a surprise -­ unlike the widespread maria on the nearside, basaltic volcanism was restricted to a relatively few, smaller regions on the farside, and the battered highlands crust dominated. A different world from what we saw from Earth.

Of course, the cause of the farside/nearside asymmetry is an interesting scientific question. Past studies have shown that the crust on the farside is thicker, likely making it more difficult for magmas to erupt on the surface, limiting the amount of farside mare basalts. Why is the farside crust thicker? That is still up for debate, and in fact several presentations at this week's Lunar and Planetary Science Conference attempt to answer this question.

The Clementine mission obtained beautiful mosaics with the sun high in the sky (low phase angles), but did not have the opportunity to observe the farside at sun angles favorable for seeing surface topography. This WAC mosaic provides the most complete look at the morphology of the farside to date, and will provide a valuable resource for the scientific community. And it's simply a spectacular sight!

The Lunar Reconnaissance Orbiter Camera (LROC) Wide Angle Camera (WAC) is a push-frame camera that captures seven color bands (321, 360, 415, 566, 604, 643, and 689 nm) with a 57-km swath (105-km swath in monochrome mode) from a 50 km orbit. One of the primary objectives of LROC is to provide a global 100 m/pixel monochrome (643 nm) base map with incidence angles between 55°-70° at the equator, lighting that is favorable for morphological interpretations. 
Each month, the WAC provides nearly complete coverage of the Moon under unique lighting. As an added bonus, the orbit-to-orbit image overlap provides stereo coverage. Reducing all these stereo images into a global topographic map is a big job, and is being led by LROC Team Members from the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR). Several preliminary WAC topographic products have appeared in LROC featured images over the past year (Orientale basin, Sinus Iridum). 
For a sneak preview of the WAC global DEM with the WAC global mosaic, view a rotating composite moon (70 MB video from ASU's LROC website). The WAC topographic dataset will be completed and released later this year.

The global mosaic released today is comprised of over 15,000 WAC images acquired between November 2009 and February 2011. The non-polar images were map projected onto the GLD100 shape model (WAC derived 100 m/pixel DTM), while polar images were map projected on the LOLA shape model. In addition, the LOLA derived crossover corrected ephemeris, and an improved camera pointing, provide accurate positioning (better than 100 m) of each WAC image.

As part of the March 2011 PDS release, the LROC team posted the global map in ten regional tiles. Eight of the tiles are equirectangular projections that encompass 60° latitude by 90° longitude. In addition, two polar stereographic projections are available for each pole from ±60° to the pole. These reduced data records (RDR) products will be available for download on March 15, 2011. As the mission progresses, and our knowledge of the lunar photometric function increases, improved and new mosaics will be released! Work your way around the moon with these six orthographic projections constructed from WAC mosaics. The nearside view linked below is different from that released on 21 February.


images of the moon Six orthographic views of the Moon created from the new WAC global mosaic. From upper left to lower right the central longitude is 0°, 60°, 120°, 180°, 240°, 300°. Credit: NASA/Goddard/Arizona State University.

NASA Kepler Mission Manager Update - Another 93 Gigabits of Data Added to the Archive

image
During a regularly scheduled science data download on Tuesday, April 26, the project team reoriented the Kepler spacecraft to downlink data from its solid-state recorder (SSR). All data collected since March 20 was returned successfully. The Quarter 9, Month 1 science data collection download now is complete.

Communications with Kepler while it is in the science attitude is accomplished using a low gain antenna on the spacecraft that operates on X-band frequency. To return all the science and engineering data that has been stored on the SSR, a high-gain antenna (HGA) operating in Ka-band frequency is used. The HGA must be pointed at Earth to support the high rate downlink (4.3 Mbps). This temporarily prohibits the spacecraft from pointing at the science field-of-view.

The monthly activity includes collection of science calibration data; turning the HGA toward Earth; and, playing back the SSR data - approximately 45 minutes for engineering data and another 5.25 hours for 37 days of science data. The number of days in each month's science set varies a bit due to Deep Space Network, or DSN, availability and other scheduling constraints. A total of 93 gigabits of data was downloaded in approximately six hours before reorienting the spacecraft to science attitude.

In order to return to the fine point attitude control, which is the highest pointing stability and what is required for science, the project team must wait for the spacecraft to return to the thermal condition it was in before the break. When the spacecraft is turned to a different attitude, the sun shines on different parts of the structure, which causes it to warp ever so slightly. This slight warping means that the angle between the star trackers and the telescope line of sight is a bit off. 

When it's maneuvered back to the science attitude, it takes time to settle back to its original shape. Until the spacecraft has thermally settled, the telescope will not be aligned with its guide stars well enough for us to transition to fine point. This can take eight hours or more. This month's activity went very well, and the total science break, which includes the collection of calibration data, was about 17 hours. The monthly budget is 20 hours.

The data is downloaded via NASA's DSN operated by the Jet Propulsion Laboratory (JPL), a division of the California Institute of Technology (Caltech) in Pasadena, Calif. From the DSN, the data flows to the Mission Operations Center in Boulder, Colo., and on to the Data Management Center in Baltimore, Md. The raw pixels are archived at the Data Management Center and then transmitted to the Kepler Science Operations Center (SOC) at NASA's Ames Research Center in Moffett Field, Calif.

The data has arrived at the SOC and will be processed this week.

Kepler is currently 32 million kilometers from Earth, collecting science data at the Spring attitude (the angular orientation of the spacecraft), in its 9th quarter of operations. All subsystems are operating normally. The next download of science data is scheduled for May 25.

TRMM Maps a Wet Spring, 2011 for the Central U.S.

NASA's Tropical Rainfall Measuring Mission satellite has been keeping track of the drenching rainfall that has been occurring in the central U.S. this springtime, and a newly created rain map from that data from April to May 4, 2011 shows those soaked areas.

A combination of heavy rains and a large snow melt has put parts of the central U.S. at risk for record flooding this spring with several locations along the Mississippi already at or near record levels. One likely culprit is La Niña. Despite the fact that the current La Niña appears to be winding down, its effects in the atmosphere can persist for a while. Furthermore, although not every La Niña brings major flooding to the region, La Niña's are conducive for above-normal rainfall from East Texas and northern Louisiana up through Arkansas and the Tennessee and Ohio Valleys with below-normal rainfall across Texas, southern Louisiana and Florida.

Rainfall anomalies were created in this rainfall map for the period April 4 to May 4, 2011 for the eastern two thirds of the country.

TMPA rainfall anomalies were created in this rainfall map for the period April 4 to May 4, 2011 for the eastern two thirds of the country. The anomalies were constructed by computing the average rainfall rate over the period and then subtracting the 10-year average rate for the same period. Credit: NASA/SSAI, Hal Pierce

During La Niña, below-normal sea surface temperatures occur in the equatorial East Pacific and above-normal temperatures in the West Pacific. This pattern leads to enhanced tropical thunderstorm activity over the West Pacific, which in turn can influence the weather in middle latitudes by shifting the jet stream pattern. On average, La Niña's favor an upper-level trough over the Midwest with the jet stream dipping down out of the northern Rockies and flowing west-to-east across the central Mississippi and Ohio Valleys before heading back up over the Northeast. This pattern steers developing low pressure systems across the Plains and central Mississippi into the Tennessee and Ohio Valleys. These areas of low pressure provide the focus for showers and storms while drawing warm moist air up from the Gulf of Mexico, resulting in enhanced rainfall across the central part of the country.

The main objective of the Tropical Rainfall Measuring Mission or TRMM satellite is to measure rainfall over the global Tropics. TRMM measures rainfall using a combination of passive microwave and active radar sensors. For expanded coverage, TRMM can be used to calibrate rainfall estimates from other satellites. The TRMM-based, near-real time Multi-satellite Precipitation Analysis (TMPA) at the NASA Goddard Space Flight Center, Greenbelt, Md. provides rainfall estimates over the global Tropics.

TMPA rainfall anomalies were created in a rainfall map for the period April 4 to May 4, 2011 for the eastern two thirds of the country. The anomalies were constructed by computing the average rainfall rate over the period and then subtracting the 10-year average rate for the same period. The resulting pattern shows a broad area of above-normal rainfall (shown in green and blue) stretching from eastern Oklahoma across the central Mississippi Valley and up into the lower Ohio Valley with below-normal rainfall along the northern Gulf Coast. This rainfall pattern is consistent with a La Niña.

In addition to rainfall, this type of jet stream pattern can lead to strong storms by allowing strong jet stream winds to override warm moist air from the Gulf as was evidenced by the recent tornado outbreak. In fact, some of the biggest tornado outbreaks, including the previous record "Super Outbreak" in 1974, have occurred during La Niña's.

TRMM is a joint mission between NASA and the Japanese space agency JAXA.
 
Steve Lang
SSAI/NASA Goddard Space Flight Center

Dawn Reaches Milestone Approaching Asteroid Vesta

Artist's concept of Dawn NASA's Dawn spacecraft, illustrated in this artist's concept, is propelled by ion engines. Image credit: NASA/JPL

› Journal entry on approach phase

PASADENA, Calif. – NASA's Dawn spacecraft has reached its official approach phase to the asteroid Vesta and will begin using cameras for the first time to aid navigation for an expected July 16 orbital encounter. The large asteroid is known as a protoplanet – a celestial body that almost formed into a planet.

At the start of this three-month final approach to this massive body in the asteroid belt, Dawn is 1.21 million kilometers (752,000 miles) from Vesta, or about three times the distance between Earth and the moon. During the approach phase, the spacecraft's main activity will be thrusting with a special, hyper-efficient ion engine that uses electricity to ionize and accelerate xenon. The 12-inch-wide ion thrusters provide less thrust than conventional engines, but will provide propulsion for years during the mission and provide far greater capability to change velocity.

"We feel a little like Columbus approaching the shores of the New World," said Christopher Russell, Dawn principal investigator, based at the University of California in Los Angeles (UCLA). "The Dawn team can't wait to start mapping this Terra Incognita."

Dawn previously navigated by measuring the radio signal between the spacecraft and Earth, and used other methods that did not involve Vesta. But as the spacecraft closes in on its target, navigation requires more precise measurements. By analyzing where Vesta appears relative to stars, navigators will pin down its location and enable engineers to refine the spacecraft's trajectory. Using its ion engine to match Vesta's orbit around the sun, the spacecraft will spiral gently into orbit around the asteroid. When Dawn gets approximately 16,000 kilometers (9,900 miles) from Vesta, the asteroid's gravity will capture the spacecraft in orbit.

"After more than three-and-a-half years of interplanetary travel, we are finally closing in on our first destination," said Marc Rayman, Dawn's chief engineer, at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "We're not there yet, but Dawn will soon bring into focus an entire world that has been, for most of the two centuries scientists have been studying it, little more than a pinpoint of light."

Scientists will search the framing camera images for possible moons around Vesta. None of the images from ground-based and Earth-orbiting telescopes have seen any moons, but Dawn will give scientists much more detailed images to determine whether small objects have gone undiscovered.

The gamma ray and neutron detector instrument also will gather information on cosmic rays during the approach phase, providing a baseline for comparison when Dawn is much closer to Vesta. Simultaneously, Dawn's visible and infrared mapping spectrometer will take early measurements to ensure it is calibrated and ready when the spacecraft enters orbit around Vesta.

Dawn's odyssey, which will take it on a journey of 4.8-billion kilometers (3-billion miles), began on Sept. 27, 2007, with its launch from Cape Canaveral Air Force Station in Florida. It will stay in orbit around Vesta for one year. After another long cruise phase, Dawn will arrive at its second destination, an even more massive body in the asteroid belt, called Ceres, in 2015.

These two icons of the asteroid belt will help scientists unlock the secrets of our solar system's early history. The mission will compare and contrast the two giant bodies, which were shaped by different forces. Dawn's science instrument suite will measure surface composition, topography and texture. In addition, the Dawn spacecraft will measure the tug of gravity from Vesta and Ceres to learn more about their internal structures.

The Dawn mission to Vesta and Ceres is managed by JPL for NASA's Science Mission Directorate in Washington. Dawn is a project of SMD's Discovery Program, which is managed by NASA's Marshall Space Flight Center in Huntsville, Ala. UCLA is responsible for overall Dawn mission science. Orbital Sciences Corp. of Dulles, Va., designed and built the Dawn spacecraft. 

The framing cameras have been developed and built under the leadership of the Max Planck Institute for Solar System Research in Katlenburg-Lindau in Germany, with significant contributions by the German Aerospace Center (DLR) Institute of Planetary Research in Berlin, and in coordination with the Institute of Computer and Communication Network Engineering in Braunschweig. The framing camera project is funded by NASA, the Max Planck Society and DLR.

JPL is a division of the California Institute of Technology, Pasadena.

For more information about Dawn, visit: http://www.nasa.gov/dawn and http://dawn.jpl.nasa.gov

To learn more about Dawn's approach phase, read the latest Dawn Journal at http://blogs.jpl.nasa.gov/2011/05/dawn-begins-its-vesta-phase/


Jia-Rui C. Cook 818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif.
jia-rui.c.cook@jpl.nasa.gov