Aug 26 2015
From The Space Library
Release M15-129 NASA Television to Air Launch of Next International Space Station Crew
The next three crew members bound for the International Space Station are set to launch to the orbital outpost Wednesday, Sept. 2.
NASA Television launch coverage will begin at 11:45 p.m. EDT on Tuesday, Sept. 1.
Sergei Volkov of the Russian Federal Space Agency (Roscosmos), Andreas Mogensen of ESA (European Space Agency) and Aidyn Aimbetov of the Kazakh Space Agency will launch from the Baikonur Cosmodrome in Kazakhstan at 12:37 a.m. Wednesday (10:37 a.m. Baikonur time). Mogensen and Aimbetov are short duration crew members while Volkov will spend six months on the orbital complex.
The trio will travel in a Soyuz spacecraft, which will rendezvous with the space station and dock two days later to the Poisk module at 3:42 a.m. on Friday, Sept. 4. NASA TV coverage of docking will begin at 3 a.m.
The hatches between the Soyuz and station will be opened at about 6:15 a.m. on Sept. 4, at which time the newly arrived crew members will be greeted by Expedition 44 Commander Gennady Padalka of Roscosmos, as well as Flight Engineers Oleg Kononenko and Mikhail Kornienko of Roscosmos, Scott Kelly and Kjell Lindgren of NASA, and Kimiya Yui of the Japan Aerospace Exploration Agency. NASA TV coverage of the hatch opening will begin at 5:45 a.m.
This will be the first time nine crew members are aboard the station simultaneously since November 2013. Padalka, Mogensen and Aimbetov will return to Earth on Saturday, Sept. 12, leaving Kelly in command of Expedition 45. The change of command ceremony in which Padalka will hand over command of the space station to Kelly will be broadcast on NASA TV on Saturday, Sept. 5 at 2:40 p.m.
Kelly and Kornienko will return in March 2016 after spending a year on the station collecting valuable biomedical data that will improve our understanding of the effects of long duration space travel and aid in NASA’s journey to Mars.
Together, the Expedition 45 crew members will continue the several hundred experiments in biology, biotechnology, physical science and Earth science currently underway and scheduled to take place aboard humanity’s only orbiting laboratory.
Release 15-175 NASA Invites Student Teams to Participate in Underwater Research
NASA is offering undergraduate students an opportunity to work in the deep end of spacewalk training through the Micro-g Neutral Buoyancy Experiment Design Teams (Micro-g NExT) activity.
Micro-g NExT challenges students to design and build prototypes of spacewalking tools to be used by NASA astronauts for spacewalk training in the Neutral Buoyancy Laboratory (NBL) at NASA’s Johnson Space Center in Houston.
The deadline for proposal submission is Oct. 26. Student selections will be announced in December. Applicants must be U.S. citizens, and full-time undergraduate students enrolled in an accredited U.S. institution of higher learning (junior college, community college, or university) at the time the proposal is submitted.
Teams will be selected to participate in the experiential/hands-on learning portion and will travel to Houston to have their prototype tested in the simulated microgravity environment of the NBL— a 6.2 million gallon indoor pool where NASA astronauts perform complex training activities in advance of their assigned space missions.
Micro-g NExT is managed by Johnson’s Office of Education with support from the agency’s Human Exploration and Operations Mission Directorate. The project encourages research and development in new technologies and engages students in real-world engineering and problem-solving concepts that may be needed on future exploration missions, including to an asteroid and Mars. The activity also supports the use of NASA's unique missions and facilities to engage and encourage students to pursue science, technology, engineering and math (STEM) careers.
Release 15-174 NASA Science Zeros in on Ocean Rise: How Much? How Soon?
Seas around the world have risen an average of nearly 3 inches since 1992, with some locations rising more than 9 inches due to natural variation, according to the latest satellite measurements from NASA and its partners. An intensive research effort now underway, aided by NASA observations and analysis, points to an unavoidable rise of several feet in the future.
Members of NASA’s new interdisciplinary Sea Level Change Team will discuss recent findings and new agency research efforts during a media teleconference today at 12:30 p.m. EDT. NASA will stream the teleconference live online.
The question scientists are grappling with is how quickly will seas rise?
“Given what we know now about how the ocean expands as it warms and how ice sheets and glaciers are adding water to the seas, it’s pretty certain we are locked into at least 3 feet of sea level rise, and probably more,” said Steve Nerem of the University of Colorado, Boulder, and lead of the Sea Level Change Team. “But we don't know whether it will happen within a century or somewhat longer.”
Team scientists will discuss a new visualization based on 23 years of sea level data – the entire record of available satellite data -- which reveals changes are anything but uniform around the globe. The record is based on data from three consecutive satellite missions, the first a collaboration between NASA and the French space agency, Centre National d'Études Spatiales, launched in 1992. The next in the series is Jason-3, led by the National Oceanic and Atmospheric Administration (NOAA) with participation by NASA, CNES and the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT).
In 2013, the United Nations Intergovernmental Panel on Climate Change (IPCC) issued an assessment based on a consensus of international researchers that stated global sea levels would likely rise from 1 to 3 feet by the end of the century. According to Nerem, new research available since this report suggests the higher end of that range is more likely, and the question remains how that range might shift upward.
The data reveal the height of the sea surface is not rising uniformly everywhere. Regional differences in sea level rise are dominated by the effects of ocean currents and natural cycles such as the Pacific Decadal Oscillation (PDO). But, as these natural cycles wax and wane, they can have major impacts on local coastlines.
“Sea level along the west coast of the United States has actually fallen over the past 20 years because long-term natural cycles there are hiding the impact of global warming,” said Josh Willis, an oceanographer at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California. “However, there are signs this pattern is changing. We can expect accelerated rates of sea level rise along this coast over the next decade as the region recovers from its temporary sea level ‘deficit.’”
Scientists estimate that about one-third of sea level rise is caused by expansion of warmer ocean water, one-third is due to ice loss from the massive Greenland and Antarctic ice sheets, and the remaining third results from melting mountain glaciers. But, the fate of the polar ice sheets could change that ratio and produce more rapid increases in the coming decades.
The Greenland ice sheet, covering 660,000 square miles -- nearly the area of Alaska -- shed an average of 303 gigatons of ice a year over the past decade, according to satellite measurements. The Antarctic ice sheet, covering 5.4 million square miles --larger than the United States and India combined -- has lost an average of 118 gigatons a year.
“We’ve seen from the paleoclimate record that sea level rise of as much as 10 feet in a century or two is possible, if the ice sheets fall apart rapidly,” said Tom Wagner, the cryosphere program scientist at NASA Headquarters in Washington. “We’re seeing evidence that the ice sheets are waking up, but we need to understand them better before we can say we’re in a new era of rapid ice loss.”
Although Antarctica’s contribution to sea level rise currently is much smaller than that of Greenland, recent research indicates this could change in the upcoming century. In 2014, two West Antarctica studies focused on the acceleration of the glaciers in the Amundsen Sea sector showed its collapse is underway.
East Antarctica’s massive ice sheet remains the primary unknown in sea level rise projections. Though it appears to be stable, a recent study found under a major glacier two deep troughs that could draw warm ocean water to the base of the glacier, causing it to melt.
“The prevailing view among specialists has been that East Antarctica is stable, but we don’t really know,” said glaciologist Eric Rignot of the University of California Irvine and JPL. “Some of the signs we see in the satellite data right now are red flags that these glaciers might not be as stable as we once thought. There’s always a lot of attention on the changes we see now, but as scientists our priority needs to be on what the changes could be tomorrow.”
One of the keys to understanding future rates of ice loss is determining the role ocean currents and ocean temperatures play in melting the ice sheets from below its edges. A new six-year NASA field campaign took to the waters around Greenland this summer to probe how warming ocean waters are triggering Greenland glacier degradation. The Oceans Melting Greenland (OMG) project is taking coastal ocean temperature measurements, observing glacial thinning at the ice’s edge, and producing the first high-resolution maps of the seafloor, fjords and canyons in the continental shelf surrounding Greenland.
NASA uses the vantage point of space to increase our understanding of our home planet, improve lives, and safeguard our future. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records. The agency freely shares this unique knowledge and works with institutions around the world to gain new insights into how our planet is changing.
Chandra Data Suggest Giant Collision Triggered “Radio Phoenix”
Astronomers have found evidence for a faded electron cloud “coming back to life,” much like the mythical phoenix, after two galaxy clusters collided. This “radio phoenix,” so-called because the high-energy electrons radiate primarily at radio frequencies, is found in Abell 1033. The system is located about 1.6 billion light years from Earth.
By combining data from NASA’s Chandra X-ray Observatory, the Westerbork Synthesis Radio Telescope in the Netherlands, NSF’s Karl Jansky Very Large Array (VLA), and the Sloan Digital Sky Survey (SDSS), astronomers were able to recreate the scientific narrative behind this intriguing cosmic story of the radio phoenix.
Galaxy clusters are the largest structures in the Universe held together by gravity. They consist of hundreds or even thousands of individual galaxies, unseen dark matter, and huge reservoirs of hot gas that glow in X-ray light. Understanding how clusters grow is critical to tracking how the Universe itself evolves over time.
Astronomers think that the supermassive black hole close to the center of Abell 1033 erupted in the past. Streams of high-energy electrons filled a region hundreds of thousands of light years across and produced a cloud of bright radio emission. This cloud faded over a period of millions of years as the electrons lost energy and the cloud expanded.
The radio phoenix emerged when another cluster of galaxies slammed into the original cluster, sending shock waves through the system. These shock waves, similar to sonic booms produced by supersonic jets, passed through the dormant cloud of electrons. The shock waves compressed the cloud and re-energized the electrons, which caused the cloud to once again shine at radio frequencies.
A new portrait of this radio phoenix is captured in this multiwavelength image of Abell 1033. X-rays from Chandra are in pink and radio data from the VLA are colored green. The background image shows optical observations from the SDSS. A map of the density of galaxies, made from the analysis of optical data, is seen in blue. Mouse over the image to see the location of the radio phoenix.
The Chandra data show hot gas in the clusters, which seems to have been disturbed during the same collision that caused the re-ignition of radio emission in the system. The peak of the X-ray emission is seen to the south (bottom) of the cluster, perhaps because the dense core of gas in the south is being stripped away by surrounding gas as it moves. The cluster in the north may not have entered the collision with a dense core, or perhaps its core was significantly disrupted during the merger. On the left side of the image, a so-called wide-angle tail radio galaxy shines in the radio. The lobes of plasma ejected by the supermassive black hole in its center are bent by the interaction with the cluster gas as the galaxy moves through it.
Astronomers think they are seeing the radio phoenix soon after it had reborn, since these sources fade very quickly when located close to the center of the cluster, as this one is in Abell 1033. Because of the intense density, pressure, and magnetic fields near the center of Abell 1033; a radio phoenix is only expected to last a few tens of millions of years.
A paper describing these results was published in a recent issue of the Monthly Notices of the Royal Astronomical Society and a preprint is available online. The authors are Francesco de Gasperin from the University of Hamburg, Germany; Georgiana Ogrean and Reinout van Weeren from the Harvard-Smithsonian Center for Astrophysics; William Dawson from the Lawrence Livermore National Lab in Livermore, California; Marcus Brüggen and Annalisa Bonafede from the University of Hamburg, Germany, and Aurora Simionescu from the Japan Aerospace Exploration Agency in Sagamihara, Japan.
NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.
