Feb 5 2018

From The Space Library

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Current revision

RELEASE 18-007 Combined Optics, Science Instruments of NASA’s James Webb Space Telescope Arrive in California

The Space Telescope Transporter for Air, Road and Sea (STTARS), a specially designed shipping container that held the optical telescope and integrated science instrument module (OTIS) of NASA’s James Webb Space Telescope, is unloaded from a U.S. military C-5 Charlie aircraft at Los Angeles International Airport (LAX) on Feb. 2, 2018.

The two halves of NASA’s James Webb Space Telescope now reside at Northrop Grumman Aerospace Systems in Redondo Beach, California, where they will come together to form the complete observatory.

Webb’s optical telescope and integrated science instrument module (OTIS) arrived at Northrop Grumman Feb. 2, from NASA’s Johnson Space Center in Houston, where it successfully completed cryogenic testing.

“This is a major milestone,” said Eric Smith, director of the James Webb Space Telescope Program at NASA. “The Webb observatory, which is the work of thousands of scientists and engineers across the globe, will be carefully tested to ensure it is ready to launch and enable scientists to seek the first luminous objects in the universe and search for signs of habitable planets.”

In preparation for leaving Johnson, OTIS was placed inside a specially designed shipping container called the Space Telescope Transporter for Air, Road and Sea (STTARS). The container then was loaded onto a U.S. military C-5 Charlie aircraft at Ellington Field Joint Reserve Base, just outside of Johnson. From there, OTIS took an overnight flight to Los Angeles International Airport. After arrival, OTIS was driven from the airport to Northrop Grumman’s Space Park facility.

“It’s exciting to have both halves of the Webb observatory – OTIS and the integrated spacecraft element – here at our campus,” said Scott Willoughby, vice president and program manager for Webb at Northrop Grumman. “The team will begin the final stages of integration of the world’s largest space telescope.”

During this summer, OTIS will undergo additional testing before being combined with the spacecraft element to form the complete Webb observatory. Once the telescope is fully integrated, the entire observatory will undergo more tests during what is called observatory-level testing. Webb is scheduled to launch from Kourou, French Guiana, in 2019.

The James Webb Space Telescope is the world’s premier infrared space observatory of the next decade. Webb will help humanity solve the mysteries of our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.

RELEASE 18-006 New NASA Space Sensors to Address Key Earth Science Questions

Why is the Arctic warming faster than the rest of the planet? Does mineral dust warm or cool the atmosphere? NASA has selected two new, creative research proposals to develop small, space-based instruments that will tackle these fundamental questions about our home planet and its environment.

The Polar Radiant Energy in the Far Infrared Experiment (PREFIRE) will fly a pair of small CubeSat satellites to probe a little-studied portion of the radiant energy emitted by Earth for clues about Arctic warming, sea ice loss, and ice-sheet melting. Tristan L’Ecuyuer of the University of Wisconsin, Madison, is the principal investigator.

The Earth Surface Mineral Dust Source Investigation (EMIT) will use a sensor mounted to the exterior of the International Space Station to determine the mineral composition of natural sources that produce dust aerosols around the world. By measuring in detail which minerals make up the dust, EMIT will help to answer the essential question of whether this type of aerosol warms or cools the atmosphere. Robert Green of NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, is the principal investigator.

These two instruments were competitively selected from 14 proposals considered under NASA's fourth Earth Venture Instrument opportunity. Earth Venture investigations are small, targeted science investigations that complement NASA's larger missions. The National Research Council recommended in 2007 that NASA undertake this type of regularly solicited, science-based, quick-turnaround project. The council’s recently released decadal survey recommended the continuance of the program.

"PREFIRE and EMIT make innovative use of technologies first developed by NASA for planetary missions to address important, longstanding questions about Earth,” said Michael Freilich, director of the Earth Science Division at NASA Headquarters in Washington.

The Arctic helps to regulate Earth’s overall temperature by radiating back into space much of the excess energy from the Sun that is absorbed at lower latitudes. Current satellite instruments do not detect all of the wavelengths of this energy radiating from our planet. PREFIRE will fill in the current data gap at far-infrared wavelengths, collecting information that will help scientists diagnose the impact of this outgoing radiation on the Arctic region’s energy balance.

PREFIRE will fly miniaturized thermal infrared spectrometers on two CubeSat satellites, each about the size of a loaf of bread. The sensors are based on technology previously flown on the Mars Climate Sounder, an instrument on NASA's Mars Reconnaissance Orbiter. The CubeSats will orbit Earth’s poles to measure far-infrared emissions and how they change throughout the day and over seasons. The observations will allow scientists to assess how changes in thermal infrared emissions at the top of Earth’s atmosphere are related to changes in cloud cover and surface conditions below, such as the amount of sea ice and meltwater on the surface of the ice.

The PREFIRE team brings together expertise in remote sensing, Earth system modeling, and Arctic Ice. JPL and the Space Dynamics Laboratory of North Logan, Utah, are mission partners.

The composition of airborne dust particles is largely unknown, but it is a critical factor in determining whether mineral-based dust has a cooling or warming effect on the atmosphere. Scientists do not currently have a global inventory of the natural mineral sources of dust, and as a result the global impacts of dust on weather, atmospheric circulation, and other aspects of Earth’s environment are not well established.

EMIT’s hyperspectral instrument will measure the different wavelengths of light emitted by minerals on the surface of deserts and other dust sources to determine their composition. The EMIT sensor is based in part on NASA’s Moon Mineralogy Mapper instrument aboard the Indian Space Research Organization's Chandrayaan-1 spacecraft. 2003 satellite image shows a large dust plume blowing off the Sahara Desert and out over the Atlantic Ocean A sensor mounted to the exterior of the International Space Station will determine the mineral composition of natural sources that produce dust aerosols around the world to answer the question of whether this type of aerosol warms or cools the atmosphere. This 2003 satellite image shows a large dust plume blowing off the Sahara Desert and out over the Atlantic Ocean. Credits: NASA

The EMIT team brings together broad expertise that covers mineral measurements, soil science, remote-sensing of surface properties, and Earth system modeling. The project’s modeling component will use the data collected to advance our understanding of the role of atmospheric dust in Earth’s climate and better predict how it can be expected to change in the future.

Earth Venture missions provide an innovative approach to address Earth science research with regular windows of opportunity to accommodate new scientific priorities. The missions are managed by NASA’s Earth System Science Pathfinder program, located at NASA’s Langley Research Center in Hampton, Virginia, for the agency’s Science Mission Directorate.

The first Earth Venture Instruments headed to space are preparing for launch within the next year. The Global Ecosystem Dynamics Investigation (GEDI) and the ECOsystem Spaceborne Thermal Radiometer Experiment on Space Station (ECOSTRESS) will measure the distributions, canopy heights, and changes in global vegetation from the space station, providing insights into how forests and ecosystems are affected by changes in water availability and other environmental and human factors.