jeudi 13 janvier 2011
A First Look at Flight in 2025
NASA logo.
01.13.11
In late 2010, NASA awarded contracts to three teams — Lockheed Martin, Northrop Grumman, The Boeing Company — to study advanced concept designs for aircraft that could take to the skies in the year 2025.
At the time of the award, the team gave NASA a sneak peek of the particular design they plan to pursue.
Image above: Artist's concept of an aircraft that could enter service in 2025 from the team led by Northrop Grumman. Credit: NASA / Northrop Grumman.
Each design looks very different, but all final designs have to meet NASA's goals for less noise, cleaner exhaust and lower fuel consumption. Each aircraft has to be able to do all of those things at the same time, which requires a complex dance of tradeoffs between all of the new advanced technologies that will be on these vehicles.
Image above: Artist's concept of an aircraft that could enter service in 2025 from the team led by The Boeing Company. Image credit: NASA / The Boeing Company.
The proposed aircraft will also have to operate safely in a more modernized air traffic management system.
And each design has to fly up to 85 percent of the speed of sound; cover a range of approximately 7,000 miles; and carry between 50,000 and 100,000 pounds of payload, either passengers or cargo.
Image above: Artist's concept of an aircraft that could enter service in 2025 from the team led by Lockheed Martin. Image credit: NASA / Lockheed Martin.
For the rest of this year, each team will be exploring, testing, simulating, keeping and discarding innovations and technologies to make their design a winner.
How different will the final designs look from these initial glimpses? Check back and see.
Read About Aircraft Designs for 2035: http://www.nasa.gov/topics/aeronautics/features/future_airplanes.html
Images (mentioned), Text, Credit: NASA.
Greetings, Orbiter.ch
NASA Updates Shuttle Target Launch Dates For Two Flights
NASA - Space Shuttle Program 1981-2011 patch.
Jan. 13, 2011
NASA is targeting 4:50 p.m. EST on Thursday, Feb. 24, for the launch of space shuttle Discovery's STS-133 mission to the International Space Station. The liftoff of shuttle Endeavour's STS-134 flight is planned for 7:48 p.m. EDT on April 19, from NASA's Kennedy Space Center in Florida.
The target dates were selected Thursday during the Space Shuttle Program's weekly Program Requirements Control Board meeting.
Space Shuttle, aerial view
NASA sets official launch dates for each shuttle mission following agency Flight Readiness Reviews, which typically occur about two weeks prior to launches. All target launch dates are subject to change.
For more information about the shuttle missions and their crews, visit: http://www.nasa.gov/shuttle
The shuttle and International Space Station launch manifest is available at: http://www.nasa.gov/stationflights
Images, Text, Credit: NASA.
Cheers, Orbiter.ch
NASA Announces Backup Commander For STS-134 Mission
NASA - STS-134 Mission patch.
Jan. 13, 2011
NASA announced Thursday that astronaut Rick Sturckow will serve as a backup commander for the STS-134 space shuttle mission to facilitate continued training for the crew and support teams during STS-134 Commander Mark Kelly's absence. Kelly's wife, Congresswoman Gabrielle Giffords, was critically wounded in a shooting on Jan. 8 in Tucson, Ariz.
Kelly remains commander of the mission, which is targeted for launch on April 19 from NASA's Kennedy Space Center in Florida.
Astronaut Mark Kelly
"I recommended to my management that we take steps now to prepare to complete the mission in my absence, if necessary," Kelly said. "I am very hopeful that I will be in a position to rejoin my STS-134 crew members to finish our training."
"Mark is still the commander of STS-134," said Peggy Whitson, chief of the Astronaut Office. "He is facing many uncertainties now as he supports Gabrielle, and our goal is to allow him to keep his undistracted attention on his family while allowing preparations for the mission to progress. Designating a backup allows the crew and support team to continue training, and enables Mark to focus on his wife's care."
Astronaut Frederick Wilford Sturckow
Sturckow will begin training next week at NASA's Johnson Space Center in Houston with the rest of the STS-134 crew, which includes Pilot Greg H. Johnson, Michael Fincke, Roberto Vittori, Andrew Feustel and Greg Chamitoff. The 14-day mission to the International Space Station will deliver the Alpha Magnetic Spectrometer and spare parts that include two S-band communications antennas, a high-pressure gas tank, additional spare parts for the Dextre robot and micrometeoroid debris shields.
For more information on the STS-134 mission, visit: http://www.nasa.gov/mission_pages/shuttle/shuttlemissions/sts134/index.html
For complete biographies of the STS-134 crew, visit: http://www.jsc.nasa.gov/Bios/
Images, Text, Credits: NASA.
Greetings, Orbiter.ch
ESA - Studying Paolo’s brains
ESA - MagISStra Mission patch.
13 January 2011
ESA astronaut Paolo Nespoli, now working as a flight engineer on the International Space Station, is busy with a range of scientific experiments. The latest is peering inside his head to help understand how the human brain works.
Our brains are changing all the time – nerves are rearranging themselves and the connections between the nerve cells are reforming as the brain memorises new information, stores the old and continuously adapts to new situations.
Preparing Neurospat in the Columbus facility
New experiences, learning, physiological changes, sleep disturbance and fatigue are among the most influential factors.
Sometimes, especially after an accident or a cerebral stroke, the recover power of brain tissue is simply mind-boggling: the remaining healthy tissue can take over the functions of damaged areas.
Space is a stress factor
The weightlessness in orbit is also a big change for brains. Not only are there changes in blood circulation and other physical conditions, but the way that cognitive functions of daily life are managed also alter dramatically.
Cady gives Paolo gel injections in the scalp
Adapting to the multitudinous effects that gravity has on the human body and the way the brain deals with them is perhaps the greatest demand that the nervous system has to face in space. The increased load on the cognitive capacity is accompanied by a multitude of stresses on the brain.
On 21 December, his second full working day on the Station, Paolo set up the Neurospat experiment with assistance from crewmate Cady Coleman.
Neurospat aims to detect the brain’s mechanisms involved in the altered behaviour in weightlessness and to locate the crucial parts of the cerebral cortex.
Helping life on Earth
Specially designed display unit of the Neurospat experiment
Neurospat uses a laptop computer with a special program, a visor to focus on the computer without external visual distractions and an electroencephalograph to record brain activity.
By recording this activity, European scientists are probing the activity that underlies cognitive processes involved in four different tasks: visual-motor tracking, perception of how the body is oriented, 3D navigation and discriminating the orientation of objects.
Follow Paolo:
Follow @astro-paolo: http://www.twitter.com/astro_paolo
@astro_paolo's pictures: http://www.flickr.com/photos/magisstra
Ask Paolo on YouTube: http://www.youtube.com/watch?v=8_ikdofcUms
Images, Text, Credits: NASA / ESA / S. Corvaja, 2010.
Cheers, Orbiter.ch
'Heartbeats' From a Black Hole System
NASA - Chandra X-Ray Observatory logo.
01.13.11
This optical and infrared image from the Digitized Sky Survey shows the crowded field around the binary system GRS 1915+105 (GRS 1915 for short) located near the plane of our Galaxy. The top-left inset shows a close-up of the Chandra image of GRS 1915, and the bottom-right inset shows the remarkable "heartbeats" seen in the X-ray light from this system. Using Chandra and the Rossi X-ray Timing Explorer (RXTE), astronomers have discovered what drives these heartbeats and given new insight into the ways that black holes can regulate their intake and severely curtail their growth.
GRS 1915 contains a black hole about 14 times the mass of the sun that is feeding off material from a nearby companion star. As the material swirls toward the black hole, a disk forms. The black hole in GRS 1915 has been estimated to rotate at the maximum possible rate, allowing material in the inner disk to orbit very close to the black hole -- at a radius only 20 percent larger than the event horizon -- where the material travels at 50 percent the speed of light.
Researchers monitored this black hole system with Chandra and RXTE over a period of eight hours. As they watched, GRS 1915 gave off a short, bright pulse of X-ray light approximately every 50 seconds. This type of rhythmic cycle closely resembles an electrocardiogram of a human heart -- though at a slower pace. It was previously known that GRS 1915 can develop such heartbeats, but researchers gained new understanding into what drives the beats, and used the pulses to figure out what controls how much material the black hole consumes from the RXTE data.
The astronomers also used Chandra's high-resolution spectrograph to study the effects of this heartbeat variation on regions of the disk very far from the black hole, at distances of about 100,000 to a million times the radius of the event horizon. By analyzing the Chandra spectrum, they found a very strong wind being driven away from the outer parts of the disk. The rate of mass expelled in this wind is remarkably high, as much as 25 times the maximum rate at which matter falls onto the black hole. This massive wind drains material from the outer disk and eventually causes the heartbeat variation to shut down.
Read more/access larger images: http://chandra.harvard.edu/photo/2011/g1915/
Images, Text, Credits: X-ray: NASA / CXC / Harvard / J. Neilsen et al.; Optical: Palomar DSS2.
Greetings, Orbiter.ch
How GIOVE’s signals show way for Galileo
ESA - GALILEO-GIOVE Mission logo.
13 January 2011
Five years ago today, ESA’s GIOVE-A satellite began broadcasting Europe’s first navigation signal from space.That signal is still going strong, supporting this year’s debut of the full-scale Galileo navigation system.
Having been launched on 28 December 2005, it was two weeks later on 12 January 2006 that the first Galileo In-Orbit Validation Element satellite, GIOVE-A, began broadcasting a navigation signal synchronised with its rubidium atomic clock.
Artist impression Giove A satellite
A second satellite, GIOVE-B, adding an ultra-precise passive hydrogen maser atomic clock, was launched on 27 April 2008 and began broadcasting its own signal from medium Earth orbit on 7 May 2008.
“These signals were required to formally secure Europe’s access to the allocated Galileo frequencies, while also allowing us to assess the on-orbit functioning of the two atomic clock designs at Galileo’s heart,” said Valter Alpe, managing GIOVE operations for ESA. “Meanwhile, we could also begin to test the kind of elaborate ground processing needed for the operational Galileo system.”
All satnav systems require a dedicated ground segment to provide continuous fine-tuning of the correction data broadcast through the navigation signal. Navigation satellites must keep the time extremely accurately: their signals contain precise timings.
GIOVE-A ground track
Receivers triangulate a user’s position on Earth by calculating the distance travelled by four or more different satellite signals. Because these signals travel at the speed of light, their timings need to be ultra-accurate.
An onboard clock drifting forward or back by a billionth of a second translates into a 30 cm range error.
“The trick of the whole satellite navigation story is that the user is receiving not just the clock timing itself but also very slight corrections transmitted in the signal stating if the clock is running a few nanoseconds early or late,” said Valter.
“It takes a sophisticated ground segment to generate these corrections, but this process is essential for maintaining service accuracy.”
Spectrum from GIOVE A
A worldwide network of operational ground sensor stations is being deployed for Galileo, with the first two Galileo In-Orbit Validation (IOV) satellites due for launch this year.
Galileo sensor stations receivers will provide range measurements to be relayed back to the Galileo Control Centre in Fucino, Italy, from where navigation corrections will be formulated and transmitted. This operating principle behind the worldwide network has already been validated as part of the GIOVE project.
Five years of GIOVE's signal-in-space: a testbed for experimentation
“We set up a much simpler dedicated infrastructure for GIOVE, with an initial 11 ground stations that has since grown to 17,” explained Stefano Binda, Systems Performance Engineer for GIOVE.
“This was done through ESA’s space operations centre ESOC, in Darmstadt, Germany, and partner research institutions. But although this was done comparatively quickly and cheaply, the ground stations still need to be distributed worldwide, to guarantee the necessary depth of coverage.
GIOVE Processing Centre at ESTEC
“Each satellite needs to be seen simultaneously by at least two ground stations to be able to solve the key navigation message unknowns.
“So the network extends all the way to the Antarctic, Polynesia and Australia. Each one collects ranging and clock data, which is delivered every hour to the heart of the GIOVE ground mission segment - a facility at ESA’s Radio Navigation Laboratory based at ESTEC in Noordwijk in the Netherlands, called the GIOVE Processing Centre (GPC).”
The GPC crunches all the raw measurement data from the GIOVE ground stations to produce an updated summary of both satellites’ clocks and current orbits, as well as the ground stations’ own atomic clocks.
GIOVE architecture
This information is then passed on to the control centres of the two satellites: Guildford in the UK for GIOVE-A, Fucino in Italy for GIOVE-B, where it can then be uploaded to the satellites.
“The idea has been to really build a complete mini-navigation system, so in the end we can check the complete loop is working and get also feedback on the ground segment operations,” explained Stefano.
“We check the navigation messages produced in the GPC are the same as those retrieved from the satellites in the first place.”
This entire ground segment and all the receivers used were fully developed in Europe. The GIOVE signals are broadly similar to GPS, but reception involved some technical challenges.
GIOVE-B
For instance, GIOVE-B was the first navigation satellite to broadcast using a ‘multiplex binary offset carrier’ in one of its two channels, a special modulation that offers robust protection against signal interference and the signal reflection known as ‘multipath’.
Similar modulation has been agreed between Galileo and future versions of the GPS satellites within one shared frequency band.
The freely available nature of GIOVE signals has also supported experimentation to guarantee the interoperability of the US and European systems.
GIOVE Payload Control Interface
As an example, GPS and Galileo run on different time systems – GPS time is maintained by the US Naval Observatory, while Galileo System Time is generated by the Precise Timing facility at the Galileo Control Centre in Fucino, which is in turn cross-checked for alignment to the international Coordinated Universal Time by a combination of European timing laboratories.
For the two systems to work together, the difference between their timings must be known precisely. GIOVE signals incorporate a measurement of the current separation – called the GPS to Galileo Time Offset – on an experimental basis.
Both systems, GPS and Galileo, will broadcast an operational version of this value once Galileo is in orbit.
First two Galileo IOV satellites
The GIOVE signals-in-space have been an experimental resource for a wide variety of groups, from space agencies to receiver manufacturers and application designers, but their story appears far from over. Their atomic clocks and host satellites are showing little signs of ageing, but the mission teams are interested in monitoring future changes.
The Radio Navigation Laboratory at ESTEC includes spacecraft simulators for both satellites, as well as a cleanroom containing a replica of the GIOVE-B payload, allowing them to replicate any changes observed in GIOVE-A and –B’s behaviour.
And once Galileo reaches space these satellites will still be exceptionally valuable for future experiments such as checking effects on the system of increasing solar activity and verifying performance in the longer term including ageing effects, continuing to serve as a global testbed for Galileo service improvements.
More information:
European Commission - Galileo: http://ec.europa.eu/enterprise/policies/satnav/galileo/index_en.htm
RF Payload Systems Laboratories: http://www.esa.int/SPECIALS/Space_Engineering/SEMAWNV0EZF_0.html
GIOVE website: http://www.giove.esa.int/
Images, Text, Credits: ESA / P. Carril / RAL.
Best regards, Orbiter.ch
mercredi 12 janvier 2011
NASA Research Finds 2010 Tied For Warmest Year On Record
NASA patch.
Jan. 12, 2011
Global surface temperatures in 2010 tied 2005 as the warmest on record, according to an analysis released Wednesday by researchers at NASA's Goddard Institute for Space Studies (GISS) in New York.
The two years differed by less than 0.018 degrees Fahrenheit. The difference is smaller than the uncertainty in comparing the temperatures of recent years, putting them into a statistical tie. In the new analysis, the next warmest years are 1998, 2002, 2003, 2006 and 2007, which are statistically tied for third warmest year. The GISS records begin in 1880.
The analysis found 2010 approximately 1.34 F warmer than the average global surface temperature from 1951 to 1980. To measure climate change, scientists look at long-term trends. The temperature trend, including data from 2010, shows the climate has warmed by approximately 0.36 F per decade since the late 1970s.
Graphic above: In 2010, global temperatures continued to rise. A new analysis from the Goddard Institute for Space Studies shows that 2010 tied with 2005 as the warmest year on record, and was part of the warmest decade on record. (Graphic credit: NASA / Earth Observatory / Robert Simmon).
"If the warming trend continues, as is expected, if greenhouse gases continue to increase, the 2010 record will not stand for long," said James Hansen, the director of GISS.
The analysis produced at GISS is compiled from weather data from more than 1000 meteorological stations around the world, satellite observations of sea surface temperature and Antarctic research station measurements. A computer program uses the data to calculate temperature anomalies -- the difference between surface temperature in a given month and the average temperature for the same period during 1951 to 1980. This three-decade period acts as a baseline for the analysis.
The resulting temperature record closely matches others independently produced by the Met Office Hadley Centre in the United Kingdom and the National Oceanic and Atmospheric Administration's National Climatic Data Center.
The record temperature in 2010 is particularly noteworthy, because the last half of the year was marked by a transition to strong La Nina conditions, which bring cool sea surface temperatures to the eastern tropical Pacific Ocean.
"Global temperature is rising as fast in the past decade as in the prior two decades, despite year-to-year fluctuations associated with the El Nino-La Nina cycle of tropical ocean temperature," Hansen and colleagues reported in the Dec. 14, 2010, issue of Reviews of Geophysics.
A chilly spell also struck this winter across northern Europe. The event may have been influenced by the decline of Arctic sea ice and could be linked to warming temperatures at more northern latitudes.
Arctic sea ice acts like a blanket, insulating the atmosphere from the ocean's heat. Take away that blanket, and the heat can escape into the atmosphere, increasing local surface temperatures. Regions in northeast Canada were more than 18 degrees warmer than normal in December.
The loss of sea ice may also be driving Arctic air into the middle latitudes. Winter weather patterns are notoriously chaotic, and the GISS analysis finds seven of the last 10 European winters warmer than the average from 1951 to 1980. The unusual cold in the past two winters has caused scientists to begin to speculate about a potential connection to sea ice changes.
"One possibility is that the heat source due to open water in Hudson Bay affected Arctic wind patterns, with a seesaw pattern that has Arctic air downstream pouring into Europe," Hansen said.
For more information about GISS's surface temperature record, visit: http://data.giss.nasa.gov/gistemp/
For more information about NASA and agency programs, visit: http://www.nasa.gov
Image, Graphic, Video, Text, Credits: NASA / GISS / Goddard Space Flight Center / Earth Observatory / Robert Simmon.
Greetings, Orbiter.ch
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