NASA conducted a combined chill test and 1.9-second ignition test July 14 of the next-generation J-2X rocket engine that could help carry humans beyond low-Earth orbit to deep space.

The test at John C. Stennis Space Center is the first in a series of tests that will be conducted on the J-2X engine, which is being developed for NASA’s Marshall Space Flight Center in Huntsville, Ala., by Pratt & Whitney Rocketdyne. The ignition test on the A-2 Test Stand is the first of a series of firings over the next several months. Collected data will verify the engine functions as designed.

The J-2X engine uses liquid hydrogen and liquid oxygen as fuel, which can be mixed to generate 294,000 pounds of thrust to lift a spacecraft into low-Earth orbit or 242,000 pounds of thrust to power a spacecraft from low-Earth orbit into deep space. The engine is designed to start and restart in space.

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PASADENA, Calif. NASA’s versatile Mars Reconnaissance Orbiter, which began orbiting Mars five years ago on March 10, has radically expanded our knowledge of the Red Planet and is now working overtime.

The mission has provided copious information about ancient environments, ice-age-scale climate cycles and present-day changes on Mars.

The orbiter observes Mars’ surface, subsurface and atmosphere in unprecedented detail. The spacecraft’s large solar panels and dish antenna have enabled it to transmit more data to Earth — 131 terabits and counting, including more than 70,000 images — than all other interplanetary missions combined. Yet many things had to go well for the mission to achieve these milestones.

After a seven-month journey from Earth, the spacecraft fired its six main engines for nearly 27 minutes as it approached Mars on March 10, 2006. Mars could not capture it into orbit without this critically timed maneuver to slow the spacecraft. The orbiter’s intended path took it behind Mars, out of communication, during most of the engine burn.

“That was tense, waiting until the spacecraft came back out from behind Mars and we had contact,” recalled Dan Johnston, now the mission’s deputy project manager at NASA’s Jet Propulsion Laboratory, Pasadena, Calif.

The Mars Reconnaissance Orbiter mission met all its science goals in a two-year primary science phase. Two extensions, the latest beginning in 2010, have added to the bounty of science returns.

The mission has illuminated three very different periods of Mars history. Its observations of the heavily cratered terrains of Mars, the oldest on the planet, show that different types of ancient watery environments formed water-related minerals. Some of these would have been more favorable for life than others.

In more recent times, water appears to have cycled as a gas between polar ice deposits and lower-latitude deposits of ice and snow. Extensive layering in ice or rock probably took hundreds of thousands to millions of years to form and, like ice ages on Earth, is linked to cyclic changes in the tilt of the planet’s rotation axis and the changing intensity of sunlight near the poles.

The present climate is also dynamic, with volatile carbon dioxide and, just possibly, summertime liquid water modifying gullies and forming new streaks. With observations of new craters, avalanches and dust storms, the orbiter has shown a partially frozen world, but not frozen in time, as change continues today.

In addition to its science observations, the mission provides support for other spacecraft as they land and operate on the surface. The orbiter’s cameras captured the Phoenix Mars Lander as it parachuted to the surface in 2008 and monitored the atmosphere for dust storms that would affect Phoenix and the Mars Exploration Rovers Spirit and Opportunity. The Mars Reconnaissance Orbiter augmented NASA’s Mars Odyssey in performing relay functions for these missions.

JPL’s Phil Varghese, project manager for the Mars Reconnaissance Orbiter, said, “The spacecraft is still in excellent health. After five years at Mars, it continues with dual capabilities for conducting science observations, monitoring the Mars environment and serving as a relay.”

The orbiter has examined potential landing sites for NASA’s Mars Science Laboratory mission, which will land a rover named Curiosity at one of those sites in August 2012. “We are preparing to support the arrival of the Mars Science Laboratory and the rover’s surface operations,” Varghese said. “In the meantime, we will extend the science observations into a third Martian year.” One Mars year lasts nearly two Earth years.

The orbiter’s Mars Color Imager has produced more than four Earth years of daily global weather maps. More than 18,500 images from the High Resolution Imaging Science Experiment camera have resolved features as small as a desk in target areas scattered around the planet that, combined, cover about as much ground as Alaska. More than 36,900 images from the Context Camera cover nearly two-thirds of the surface of Mars at a resolution that allows detection of features the size of large buildings.

The Compact Reconnaissance Spectrometer for Mars has mapped minerals on more than three-fourths of the planet’s surface. The Mars Climate Sounder has monitored atmospheric temperature and aerosols with more than 59 million soundings. The Shallow Radar has checked for underground layers in more than 8,600 swaths of ground-penetrating observations.

“Each Mars year is unique, and additional coverage gives us a better chance to understand the nature of changes in the atmosphere and on the surface,” said JPL’s Rich Zurek, project scientist for the Mars Reconnaissance Orbiter. “We have already learned that Mars is a more dynamic and diverse planet than what we knew five years ago. We continue to see new things.”

JPL, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate in Washington. Lockheed Martin Space Systems, Denver, built the orbiter and partners with JPL in spacecraft operations.

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Who are we? Where do we come from? These are questions that scientists hope to find clues to by better understanding the composition and evolution of the universe.

NASA flies sophisticated space missions that can probe vast regions of space to detect spectral signatures, or fingerprints, of unknown materials.

Through the years, scientists have found that these materials are much more complicated than originally anticipated. Because conditions in space are vastly different from conditions on Earth, identifying extraterrestrial materials is extremely difficult. Recently, researchers have achieved a major milestone by adding a new capability to one of the world’s unique laboratory facilities.

Located at NASA’s Ames Research Center, Moffett Field, Calif., this specialized facility, called the Cosmic Simulation Chamber (COSmIC), integrates a variety of state-of-the-art instruments to allow scientists to form, process and monitor simulated space conditions for planetary and interstellar materials in the laboratory.

The chamber is the heart of the system. It recreates the extreme conditions that reign in space where average temperatures can be as low as 100 Kelvin (less than -170 degree Celsius!), densities are billionths of Earth’s (of the order of 10-16 – 10-17) and interstellar molecules and ions are bathed in stellar ultraviolet and visible radiation.

“The harsh conditions of space are extremely difficult to reproduce in the laboratory, and have long hindered efforts to interpret and analyze observations from space,” said Farid Salama, a space science researcher in the Astrophysics Branch at Ames.

The idea of building the COSmIC facility started as a Director’s Discretionary Fund (DDF) project initiated by Salama in 1996, and its realization represents a true success story for Ames’ DDF program. The facility resulted from collaboration between Ames space science researchers and Los Gatos research scientists as a Small Business Innovative Research (SBIR) contract awarded by NASA.

The team of space scientists and engineers, lead by Salama, designed and built this unique laboratory facility to gain a deeper understanding of the composition of our universe and of the evolution of galaxies, both major objectives of NASA’s space research program.

In 2003, Ames scientists delivered their first major milestone by coupling COSmIC with a cavity ringdown spectrometer, an extremely sensitive device that can detect the spectral fingerprint of matter at the molecular level.

Now, another major milestone has been achieved by coupling COSmIC with a time-of-flight mass spectrometer, an ultra-sensitive device that detects the mass of matter at the molecular level.

In the past, part of the problem that prevented scientists from identifying unknown matter was the inability to simulate space conditions in the gaseous state. Today, researchers can successfully simulate gas-phase environments similar to interstellar clouds, stellar envelopes or planetary atmospheres environments by expanding solids using a free jet spray.

“By doing this, we now can measure large carbon molecules, like polycyclic aromatic hydrocarbons (PAHs) and similar carbon species. This is a major accomplishment,” said Salama. “This type of new research truly pushes the frontiers of science toward new horizons, and illustrates NASA’s important contribution to science,” he added.

Scientists will use this “far out” facility to address two key problems: First, they want to identify the nature of big aerosol particles that have been detected by Cassini in the atmosphere of Saturn’s moon, Titan. The second problem they will study is the formation of interstellar grains in the outflow of carbon stars.

“We can now truly simulate in the laboratory the formation of carbon grains in the envelope of stars, a major problem in today’s astrophysics,” said Cesar Contreras a NASA Postdoctoral Program (NPP) fellow and a member of the research team.

“We begin with small carbon molecules, expose these molecules to high energy processing in COSmIC, expand them in a cold jet spray and detect them with our highly sensitive detectors,” added Contreras, who studies interstellar grains.

Funded by NASA’s Science Mission Directorate Astronomy and Physics Research and Analysis, Planetary Atmospheres and Cosmochemistry programs, this new facility will also study the very large aerosol particles that were seen by the Cassini spacecraft in the upper atmosphere of Titan.

“In the Cassini data we see evidence for large aerosols in the upper atmosphere of Titan that we plan to explain with COSmIC” said Claire Ricketts, another NASA NPP fellow and member of the team, who studies the composition of the atmosphere of Titan.

“Titan is an important body in our solar system because it helps us understand the conditions that existed on early Earth” added Ricketts. “Organic haze in the atmosphere of Titan is similar to haze in early Earth’s air.”

To understand Cassini’s data, scientists need this very powerful, very sensitive new tool. They will begin their analysis by forming molecules and species in the lab, measuring them in situ (inside their environment without disturbing them), and then trying to match their identity to Titan’s unknown aerosol molecules.

“Titan’s upper atmosphere data shows a rich spectrum. We will recreate those data in the lab and compare them to Cassini’s data. If they fit, great. If not, we will try something else. We will know when we are coming close to understanding them. We now have the right tool to do this,” said Salama.

“One day we will talk about the details and the implications of the data, but today we are celebrating the new milestone in the completion of this unique tool,” concluded Salama.

The Astrophysics and Astrochemistry Laboratory is part of the Astrophysics Branch in the Space Science and Astrobiology Division. Scientists in the Astrophysics Branch perform a wide range of astronomy and astrophysics research focusing on the development of new space, airborne and ground-based laboratory instrumentation such as COSmIC and SOFIA, as well as laboratory simulation experiments. The Ames team includes Farid Salama (POC), Claire Ricketts (NPP), Cesar Contreras (NPP) and Robert Walker.

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