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NASA & JAXA Sign Agreement For Future Earth Science Cooperation

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NASA Administrator Charles Bolden and Japan Aerospace Exploration Agency (JAXA) President Keiji Tachikawa signed an agreement defining the terms of cooperation between the agencies on the Global Precipitation Measurement (GPM) mission. The ceremony took place Thursday at the Kennedy Space Center Visitor Complex.

Building on the success of the NASA-JAXA Tropical Rainfall Measuring Mission (TRMM), GPM will begin the measurement of global precipitation, a key climate factor. It is an international collaboration that includes NASA and JAXA, with anticipated contributions of data from other international partners.

GPM is also the cornerstone of the multinational Committee on Earth Observation Satellites Precipitation Constellation that addresses one of the key observations of the Global Earth Observation System of Systems. The heart of the GPM mission is a space-borne core observatory which serves as a reference standard to unify measurements from a constellation of multinational research and operational satellites carrying microwave sensors.

GPM will provide uniformly calibrated precipitation measurements globally every 2 to 4 hours for scientific research and societal applications. For the first time, the GPM core observatory sensor measurements will make detailed observations of precipitation particle size distribution, which is key to improving the accuracy of precipitation estimates by microwave radiometers and radars.

The GPM core observatory will carry a Dual-frequency Precipitation Radar (DPR), which operates at Ku and Ka band frequencies, and a multi-channel GPM Microwave Imager (GMI) operating from 10-183 GHz. The DPR will have greater measurement sensitivity to light rain and snowfall compared to the TRMM radar. The GMI uses a set of frequencies that have been optimized to retrieve heavy, moderate, and light precipitation estimates.

Through the agreement, NASA is responsible for the GPM core observatory spacecraft bus, the GMI carried by it, and a second GMI to be flown on a partner-provided Low-Inclination Observatory. JAXA will supply the DPR for the core observatory, an H-IIA rocket for the core observatory’s launch in July 2013 and data from a conical-scanning microwave imager on the upcoming Global Change Observation Mission satellite.


Japanese Exposed Facility Attached to Kibo

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(Above) The Space Shuttle’s robotic arm grabs the Japanese Exposed Facility to move it out of Endeavour’s payload bay.

After a series of robotic arm “hand offs,” the Japanese Exposed Facility (JEF) was attached to the International Space Station’s Kibo laboratory at 7:29 p.m. EDT. The Exposed Facility is the final component of Kibo, Japan’s major contribution to the station, and will serve as a type of porch for experiments that require direct exposure to space.

The process involved three robotic arm systems. The space station and shuttle arms moved JEF from Endeavour’s payload bay to the Kibo laboratory and Kibo’s robotic arm was used to view the installation. There was a slight delay while verifying the structural latch between JEF and Kibo


First Conclusive Signature for Lunar Uranium

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Robert C. Reedy, a senior scientist at the Tucson-based Planetary Science Institute, is mapping the moon’s surface elements using data gathered by an advanced gamma-ray spectrometer (GRS) that rode aboard the Japanese Kaguya spacecraft.

The data promise to show chemical elements on the moon that have never been identified before, and Reedy and the Kaguya GRS team already have found uranium signatures in the data, an element not seen in previous moon-mapping efforts.

The uranium results were recently announced in papers presented at the 40th Lunar and Planetary Conference and at the Proceedings of the International Workshop Advances in Cosmic Ray Science. The lead authors on those papers are Prof. Naoyuki Yamashita and Prof. Nobuyuki Hasebe respectively. Both are from Japan’s Waseda University.

Earlier gamma-ray spectrometer maps from the Apollo and Lunar Prospector missions show a few of the moon’s chemical elements. But the maps constructed by Reedy and the Kaguya GRS team — using data gathered by state-of-the-art high-energy-resolution germanium detectors — are extending the earlier results and improving our understanding of the moon’s surface composition.

In addition to uranium, the Kaguya GRS data also is showing clear signatures for thorium, potassium, oxygen, magnesium, silicon, calcium, titanium and iron.

Reedy and his colleagues are using measurements from the Kaguya lunar orbiter’s GRS to construct high-quality maps of as many chemical elements as possible. Kaguya was launched in September 2007 and crashed into the moon at the end of its mission on June 10 of this year.

“We’ve already gotten uranium results, which have never been reported before,” Reedy said. “We’re getting more new elements and refining and confirming results found on the old maps. Some of these comparisons are being done with lunar elemental maps made by a Lunar Prospector team headed by PSI senior scientist Tom Prettyman.”

Reedy has been an official co-investigator on the Kaguya GRS team since 2007, and has received some support from the Japan Aerospace Exploration Agency (JAXA).

“Being selected as a co-investigator for a JAXA planetary mission is a great honor,” Reedy said.

Reedy’s continuing mapping work now is being funded for two years through NASA’s SALMON program (Stand-Alone Missions of Opportunity).

“All of the work being funded is considerably improving our knowledge of the moon’s composition and its origin and evolution,” Reedy said. It also will help scientists locate lunar resources and help with planning for future lunar missions, he added.

In addition to Reedy, the Kaguya GRS team includes Hasebe (the GRS principal investigator); Yamashita and Yuzuru Karouji, of the Waseda University in Tokyo, Japan; and Claude d’Uston and Olivier Gasnault, of the Centre d’Etude Spatiale des Rayonnements in Toulouse, France.

Source: Planetary Science Institute


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