mardi 7 mars 2017

NASA Parachute Device Could Return Small Spacecraft from Deep Space Missions












ISS - International Space Station patch.

March 7, 2017


After a two-month stay aboard the International Space Station, NASA’s Technology Educational Satellite (TechEdSat-5) that launched Dec. 9, 2016, was deployed on March 6, 2017 from the NanoRacks platform and into low-Earth orbit to demonstrate a critical technology that may allow safe return of science payloads to Earth from space.

Orbiting about 250 miles above Earth, the Exo-Brake, a tension-based, flexible braking device resembling a cross-shaped parachute, opens from the rear of the small satellite to increase the drag. This de-orbit device tests a hybrid system of mechanical struts and flexible cord with a control system that warps the Exo-Brake. This allows engineers to guide the spacecraft to a desired entry point without the use of fuel, enabling accurate landing for future payload return missions.

Small Satellite With Exo-Brake Technology Launches From International Space Station

Two additional technologies will be demonstrated on TechEdSat-5. These include the ‘Cricket’ Wireless Sensor Module, which provides a unique wireless network for multiple wireless sensors, providing real time data for TechEdSat-5.

The project team seeks to develop building blocks for larger scale systems that might enable future small or nanosatellite missions to reach the surface of Mars and other planetary bodies in the solar system.

For more information on NASA’s small spacecraft technology missions, visit: http://www.nasa.gov/cubesats

Image, Video, Text, Credits: NASA/Ames Research Center/Kimberly Williams.

Greetings, Orbiter.ch

A Mass of Viscous Flow Features












NASA - Mars Reconnaissance Orbiter (MRO) logo.

March 7, 2017


Viscous, lobate flow features are commonly found at the bases of slopes in the mid-latitudes of Mars, and are often associated with gullies.

These features are bound by ridges that resemble terrestrial moraines, suggesting that these deposits are ice-rich, or may have been ice-rich in the past. The source of the ice is unclear, but there is some thought that it is deposited from the atmosphere during periods of high obliquity, also known as axial tilt.

The flow features in this image are particularly massive and the bounding scarps appear very high standing and are layered as well. Take a look at the stereo anaglyph for a 3D view: http://static.uahirise.org/images/2017/details/cut/ESP_048913_1330.jpg

The map is projected here at a scale of 25 centimeters (9.8 inches) per pixel. [The original image scale is 25.9 centimeters (10.2 inches) per pixel (with 1 x 1 binning); objects on the order of 82 centimeters (32.2 inches) across are resolved.] North is up.

Mars Reconnaissance Orbiter (MRO)

This is a stereo pair with http://www.uahirise.org/ESP_048979_1330

The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

Mars Reconnaissance Orbiter (MRO): http://www.nasa.gov/mission_pages/MRO/main/index.html

Image, Video,  Credits: NASA/Tony Greicius/JPL-Caltech/Univ. of Arizona.


Greetings, Orbiter.ch

Second ‘colour vision’ satellite for Copernicus launched


















ESA & ARIANESPACE - Vega Flight VV09 Mission poster.


7 March 2017

Sentinel-2B liftoff

The ESA-developed Sentinel-2B satellite was launched today, doubling the coverage of high-resolution optical imaging in the Sentinel-2 mission for the European Union Copernicus environmental monitoring system.

The 1.1 tonne satellite was carried into orbit on a Vega rocket from Europe’s Spaceport in Kourou, French Guiana at 01:49 GMT on 7 March (02:49 CET; 22:49 local time, 6 March).

The first stage separated 1 min 55 sec after liftoff, followed by the second stage and fairing at 3 min 39 sec and 3 min 56 sec, respectively, and the third stage at 6 min 32 sec.

Sentinel-2B liftoff

After two more ignitions, Vega’s upper stage delivered Sentinel-2B into the targeted Sun-synchronous orbit. The satellite separated from the stage 57 min 57 sec into the flight.

Telemetry links and attitude control were then established by controllers at ESA’s operations centre in Darmstadt, Germany, allowing activation of Sentinel’s systems to begin. The satellite’s solar panel has already been deployed.

After this first ‘launch and early orbit’ phase, which typically lasts three days, controllers will begin checking and calibrating the instruments to commission the satellite. The mission is expected to begin operations in three to four months.

Sentinel-2 global coverage

“With this launch we are taking another step toward advancing the Copernicus programme, which is the most sophisticated Earth observation system in the world. And we are planning to add two more satellites to the constellation in the next months: with Sentinel-5P and Sentinel-3B,” said ESA Director General Jan Woerner.

The optical imaging Sentinel-2 mission is based on a constellation of two identical satellites: Sentinel-2A, which was launched in June 2015, and Sentinel-2B. Although launched separately, the satellites are placed in the same orbit, flying 180° apart. Every five days, the satellites jointly cover all land surfaces, large islands, and inland and coastal waters between latitudes 84°S and 84°N, optimising global coverage and data delivery.

Each Sentinel-2 satellite carries an innovative high-resolution multispectral camera with 13 spectral bands for a new perspective of land and vegetation. The combination of high-resolution, novel spectral capabilities, a field of vision covering 290 km and frequent revisit times will provide unprecedented views of Earth.  

Agricultural monitoring

Information from this mission is helping to improve agricultural practices, monitor the world’s forests, detect pollution in lakes and coastal waters, and contribute to disaster mapping.

“I have personally been involved in Copernicus since its very first day and helped shape it along its way. It is therefore extremely satisfying to see the constellation of satellites delivering data for the services we have always dreamt of,” said Josef Aschbacher, ESA’s Director of Earth Observation Programmes.

Sentinel-2B

“Sentinel-2A gets its twin brother in space with the launch of Sentinel-2B today. This allows global coverage every five days with the 13-channel high-resolution sensor, which is unprecedented in this class of satellites. I look forward to many new applications coming from Sentinel-2 now that this constellation is complete.”

Six families of Sentinel satellites will make up the core of EU’s Copernicus environmental monitoring network. An EU flagship space initiative, Copernicus provides operational information on the world’s land surfaces, oceans and atmosphere to support environmental and security policymaking, and meet the needs of citizens and service providers.

Related links:

Copernicus Programme: http://www.copernicus.eu/

Sentinel data access & technical information: https://sentinels.copernicus.eu/web/sentinel/home

Arianespace: http://www.arianespace.com/

Europe's Spaceport: http://www.esa.int/Our_Activities/Launchers/Europe_s_Spaceport

Airbus Defence and Space: http://airbusdefenceandspace.com/

CNES: http://www.cnes.fr/web/CNES-en/7114-home-cnes.php

Images, Animation, Videos, Text, Credits: ESA/ARIANESPACE/Contains modified Copernicus Sentinel data (2016), processed by ESA/ATG medialab.

Best regards, Orbiter.ch

lundi 6 mars 2017

CubeSats Deployed During Crew Ultrasound Scans











ISS - Expedition 50 Mission patch.

March 6, 2017

Four CubeSats were deployed this morning as the crew researched fluid shifts toward the head that may affect astronaut vision. Tools were also being collected and organized today ahead of possible maintenance spacewalks.

Four CubeSats were ejected Monday morning from outside Japan’s Kibo lab module using the NanoRacks CubeSat Deployer. The LEMUR-2 satellites will help monitor global ship tracking and improve weather forecasting.


Image above: Five Expedition 50 crew members gather in the Zvezda service module for mealtime. Clockwise from bottom are NASA astronaut Peggy Whitson, cosmonauts Andrey Borisenko and Oleg Novitskiy, ESA astronaut Thomas Pesquet and cosmonaut Sergey Ryzhikov. Image Credit: NASA.

Sergey Ryzhikov from Roscosmos participated in ultrasound scans of the head and neck for the long-running Fluid Shifts study. Thomas Pesquet from the European Space Agency joined Ryzhikov for the experiment to learn how to prevent upward fluid shifts that may cause lasting eye damage.

Commander Shane Kimbrough worked inside the Quest airlock today gathering spacewalk tools. Mission planners are looking at potential spacewalks to continue upgrading the International Space Station’s power systems.

Related links:

CubeSats: https://www.nasa.gov/cubesats

LEMUR-2 satellites: https://www.nasa.gov/mission_pages/station/research/experiments/2349.html

Fluid shifts: https://www.nasa.gov/mission_pages/station/research/experiments/1257.html

Quest airlock: https://www.nasa.gov/mission_pages/station/structure/elements/quest.html

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Image (mentioned), Text, Credits: NASA/Mark Garcia.

Best regards, Orbiter.ch

Scientists said an asteroid could threaten our planet...










Asteroid Watch logo.

March 6, 2017

With an antenna 305 meters in diameter, consisting of 38,778 aluminum panels with a collection area of ​​approximately 73,000 m², the Arecibo observatory has the second largest radio telescope in the world after the Chinese FAST.

The asteroid 2015 BN509

The asteroid to the form of immense peanut could, according to the observatory, one day constitute a danger to the Earth. According to the scientists, it could be that one day it could one day cross the road of the Earth and cause serious damage because of its speed, 70 000 km / h and its size, 200m wide.

Radar image of a giant, peanut-shaped asteroid may one day threaten Earth

According to Ed Rivera-Valentin, an astronomer at the University Space Research Association, the asteroid would be about 14 times the distance between Earth and the Moon, which is close to the space scale.

Researchers on the lookout

Arecibo Observatory

Scientists are therefore trying to calculate the trajectory of the asteroid and continue to monitor it. "Unlike natural disasters, an asteroid impact can be avoided," says one researcher. "That's why information gathered by Arecibo can be used by NASA to prepare a defense mission."

Related link:

Arecibo Observatory: http://www.naic.edu/

More information about asteroids and near-Earth objects can be found at:

http://cneos.jpl.nasa.gov

http://www.jpl.nasa.gov/asteroidwatch

For more information about NASA's Planetary Defense Coordination Office, visit: http://www.nasa.gov/planetarydefense

For asteroid and comet news and updates, follow AsteroidWatch on Twitter: http://twitter.com/AsteroidWatch

Asteroids: https://www.nasa.gov/mission_pages/asteroids/main/index.html

Images, Text, Credits: AFP/Wikipedia/Arecibo Observatory/NASA/NSF/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch

NASA Wants to Create the Coolest Spot in the Universe












ISS - International Space Station patch.

March 6, 2017

This summer, an ice chest-sized box will fly to the International Space Station, where it will create the coolest spot in the universe.

Inside that box, lasers, a vacuum chamber and an electromagnetic "knife" will be used to cancel out the energy of gas particles, slowing them until they're almost motionless. This suite of instruments is called the Cold Atom Laboratory (CAL), and was developed by NASA's Jet Propulsion Laboratory in Pasadena, California. CAL is in the final stages of assembly at JPL, ahead of a ride to space this August on SpaceX CRS-12.

Its instruments are designed to freeze gas atoms to a mere billionth of a degree above absolute zero. That's more than 100 million times colder than the depths of space.


Image above: Artist's concept of an atom chip for use by NASA's Cold Atom Laboratory (CAL) aboard the International Space Station. CAL will use lasers to cool atoms to ultracold temperatures. Image Credit: NASA.

"Studying these hyper-cold atoms could reshape our understanding of matter and the fundamental nature of gravity," said CAL Project Scientist Robert Thompson of JPL. "The experiments we'll do with the Cold Atom Lab will give us insight into gravity and dark energy -- some of the most pervasive forces in the universe."

When atoms are cooled to extreme temperatures, as they will be inside of CAL, they can form a distinct state of matter known as a Bose-Einstein condensate. In this state, familiar rules of physics recede and quantum physics begins to take over. Matter can be observed behaving less like particles and more like waves. Rows of atoms move in concert with one another as if they were riding a moving fabric. These mysterious waveforms have never been seen at temperatures as low as what CAL will achieve.

NASA has never before created or observed Bose-Einstein condensates in space. On Earth, the pull of gravity causes atoms to continually settle towards the ground, meaning they're typically only observable for fractions of a second.

But on the International Space Station, ultra-cold atoms can hold their wave-like forms longer while in freefall. That offers scientists a longer window to understand physics at its most basic level. Thompson estimated that CAL will allow Bose-Einstein condensates to be observable for up to five to 10 seconds; future development of the technologies used on CAL could allow them to last for hundreds of seconds.

Bose-Einstein condensates are a "superfluid" -- a kind of fluid with zero viscosity, where atoms move without friction as if they were all one, solid substance.

"If you had superfluid water and spun it around in a glass, it would spin forever," said Anita Sengupta of JPL, Cold Atom Lab project manager. "There's no viscosity to slow it down and dissipate the kinetic energy. If we can better understand the physics of superfluids, we can possibly learn to use those for more efficient transfer of energy."

Five scientific teams plan to conduct experiments using the Cold Atom Lab. Among them is Eric Cornell of the University of Colorado, Boulder and the National Institute for Standards and Technology. Cornell is one of the Nobel Prize winners who first created Bose-Einstein condensates in a lab setting in 1995.

The results of these experiments could potentially lead to a number of improved technologies, including sensors, quantum computers and atomic clocks used in spacecraft navigation.

International Space Station (ISS). Image Credit: NASA

Especially exciting are applications related to dark energy detection, said Kamal Oudrhiri of JPL, the CAL deputy project manager. He noted that current models of cosmology divide the universe into roughly 27 percent dark matter, 68 percent dark energy and about 5 percent ordinary matter.

"This means that even with all of our current technologies, we are still blind to 95 percent of the universe," Oudrhiri said. "Like a new lens in Galileo's first telescope, the ultra-sensitive cold atoms in the Cold Atom Lab have the potential to unlock many mysteries beyond the frontiers of known physics."

The Cold Atom Lab is currently undergoing a testing phase that will prepare it prior to delivery to Cape Canaveral, Florida.

"The tests we do over the next months on the ground are critical to ensure we can operate and tune it remotely while it's in space, and ultimately learn from this rich atomic physics system for years to come," said Dave Aveline, the test-bed lead at JPL.

JPL is developing the Cold Atom Laboratory, sponsored by the International Space Station Program at NASA's Johnson Space Center in Houston.

The Space Life and Physical Sciences Division of NASA's Human Exploration and Operations Mission Directorate at NASA Headquarters in Washington manages the Fundamental Physics Program.

Caltech manages JPL for NASA.

For more information about the Cold Atom Lab, visit: http://coldatomlab.jpl.nasa.gov/

The Cold Atom Lab will be the topic of two free lectures in March, one of which will be streamed live at: http://www.ustream.tv/NASAJPL2

Details about the lecture are at: http://www.jpl.nasa.gov/events/lectures_archive.php?year=2017&month=3

Images (mentioned), Text, Credits: NASA/Tony Greicius/JPL/Andrew Good.

Best regards, Orbiter.ch

Flashy First Images Arrive From NOAA’s GOES-16 Lightning Mapper












NOAA & NASA - GOES-R Mission patch.

March 6, 2017

Detecting and predicting lightning just got a lot easier. The first images from a new instrument onboard NOAA’s GOES-16 satellite are giving NOAA National Weather Service forecasters richer information about lightning that will help them alert the public to dangerous weather.


Image above: This is one hour of GOES-16's Geostationary Lightning Mapper (GLM) lightning data from Feb. 14, when GLM acquired 1.8 million images of the Earth. It is displayed over GOES-16 ABI full disk Band 2 imagery. Brighter colors indicate more lightning energy was recorded; color bar units are the calculated kilowatt-hours of total optical emissions from lightning. The brightest storm system is located over the Gulf Coast of Texas, the same storm system in the accompanying video. This is preliminary, non-operational data. Image Credits: NOAA/NASA.

The first lightning detector in a geostationary orbit, the Geostationary Lightning Mapper (GLM), is transmitting data never before available to forecasters. The mapper continually looks for lightning flashes in the Western Hemisphere, so forecasters know when a storm is forming, intensifying and becoming more dangerous. Rapid increases of lightning are a signal that a storm is strengthening quickly and could produce severe weather.

During heavy rain, GLM data will show when thunderstorms are stalled or if they are gathering strength. When combined with radar and other satellite data, GLM data may help forecasters anticipate severe weather and issue flood and flash flood warnings sooner. In dry areas, especially in the western United States, information from the instrument will help forecasters, and ultimately firefighters, identify areas prone to wildfires sparked by lightning.

First Image from GOES-16 Lightning Mapper

Video above: GOES-16's Geostationary Lightning Mapper (GLM) shows lightning over southeast Texas on Feb. 14, 2017. GLM lightning data was overlaid on Advanced Baseline Imager (ABI) cloud imagery. Frequent lightning is occurring. Houston is indicated by the green cross and green dotted lines indicate the Texas coastline. This animation, rendered at 25 frames per second, simulates what your eye might see from above the clouds. Video Credits: NOAA/NASA.

Accurate tracking of lightning and thunderstorms over the oceans, too distant for land-based radar and sometimes difficult to see with satellites, will support safe navigation for aviators and mariners.

The new mapper also detects in-cloud lightning, which often occurs five to 10 minutes or more before potentially deadly cloud-to-ground strikes. This means more precious time for forecasters to alert those involved in outdoor activities of the developing threat.

NASA successfully launched GOES-R at 6:42 p.m. EST on November 19, 2016 from Cape Canaveral Air Force Station in Florida and it was renamed GOES-16 when it achieved orbit. GOES-16 is now observing the planet from an equatorial view approximately 22,300 miles above the surface of the Earth.

NOAA’s satellites are the backbone of its life-saving weather forecasts. GOES-16 will build upon and extend the more than 40-year legacy of satellite observations from NOAA that the American public has come to rely upon.

Related link:

Geostationary Lightning Mapper (GLM): http://www.goes-r.gov/spacesegment/glm.html

Learn more about GOES-16 and all its exciting possibilities for weather forecasting improvements by visiting the GOES-16 website: https://www.nesdis.noaa.gov/GOES-16

For more information about GOES-16, visit: http://www.goes-r.gov/ or http://www.nasa.gov/goes

Image (mentioned), Video (mentioned), Text, Credits: NASA/Lynn Jenner/NOAA/Michelle Smith.

Greetings, Orbiter.ch