lundi 11 février 2013

Launch of the cargo spacecraft Progress M-18M












ROSCOSMOS logo.

11/02/2013

 Progress M-18M (P50) launch

February 11 at 18:41 MSK (Moscow time) from the launch complex of the platform 1 was launched Baikonur Launch Vehicle (ILV) Soyuz-U to transport cargo ship (THC) Progress M-18M (P50).

Russian Cargo Ship Heads to Station

According to cyclogram flight spacecraft separated from the third stage of the launch vehicle and placed into the desired orbit.

Progress Launch Profile

Docking THC Progress M-18M from the International Space Station (docking bay Pirs) is scheduled for February 12.

Progress Vehicle Events

Cargo ship - the first of a planned in 2013, must be delivered to the ISS more than 2.5 tonnes of cargo - scientific equipment and spare parts for the station, the fuel to maintain its orbit, food, water and air for the astronauts.

Original text in Russian: http://www.federalspace.ru/main.php?id=2&nid=19887

Images, Video, Text, Credits: Press Service of the Russian Federal Space Agency (Roscosmos PAO) / Roscosmos TV / NASA TV / Screen captures & Translation: Orbiter.ch Aerospace.

Greetings, Orbiter.ch

samedi 9 février 2013

Progress M-16M completed flight











ROSCOSMOS - Russian Vehicles patch.

09/02/2013

 Progress M-16M undocking from ISS

9 February at 21:05 MSK (Moscow time) in a predetermined area of ​​the South Pacific was flooding incombustible residue cargo vehicle (THC) Progress M-16M.

 Russian Cargo Ship Departs from ISS

At 20:19 MSK in accordance with the program laid down in the ship's on-board computer specialists Mission Control Center (MCC) FSUE TsNIImash, the "space truck" was added to the main engine braking, followed by the controlled reduction of the THC from orbit.

Progress M reentry profile

THC Progress M-16M was launched to the International Space Station from the Baikonur Cosmodrome August 1, 2012, to deliver the cargo of food, fuel, water and equipment.

Progress M plasma during the reentry in hi-atmosphere, seen by ISS crew

Original text in Russian: http://www.federalspace.ru/main.php?id=2&nid=19883

Images, Video, Text, Credits: Press Service of the Russian Federal Space Agency (Roscosmos PAO) / NASA / NASA TV / Roscosmos TV / G. De Chiara / Translation: Orbiter.ch Aerospace.

Cheers, Orbiter.ch

NASA Curiosity Rover Collects First Martian Bedrock Sample












NASA - Mars Science Laboratory (MSL) patch.

Feb. 9, 2013


Image above: At the center of this image from NASA's Curiosity rover is the hole in a rock called "John Klein" where the rover conducted its first sample drilling on Mars. Image credit: NASA/JPL-Caltech/MSSS.

NASA's Curiosity rover has, for the first time, used a drill carried at the end of its robotic arm to bore into a flat, veiny rock on Mars and collect a sample from its interior. This is the first time any robot has drilled into a rock to collect a sample on Mars.

The fresh hole, about 0.63 inch (1.6 centimeters) wide and 2.5 inches (6.4 centimeters) deep in a patch of fine-grained sedimentary bedrock, can be seen in images and other data Curiosity beamed to Earth Saturday. The rock is believed to hold evidence about long-gone wet environments. In pursuit of that evidence, the rover will use its laboratory instruments to analyze rock powder collected by the drill.


Animation above: An animated set of three images from NASA's Curiosity rover shows the rover's drill in action on Feb. 8, 2013, or Sol 182, Curiosity's 182nd Martian day of operations. Image credit: NASA/JPL-Caltech/MSSS.

"The most advanced planetary robot ever designed is now a fully operating analytical laboratory on Mars," said John Grunsfeld, NASA associate administrator for the agency's Science Mission Directorate. "This is the biggest milestone accomplishment for the Curiosity team since the sky-crane landing last August, another proud day for America."

For the next several days, ground controllers will command the rover's arm to carry out a series of steps to process the sample, ultimately delivering portions to the instruments inside.

"We commanded the first full-depth drilling, and we believe we have collected sufficient material from the rock to meet our objectives of hardware cleaning and sample drop-off," said Avi Okon, drill cognizant engineer at NASA's Jet Propulsion Laboratory, Pasadena, Calif.

Rock powder generated during drilling travels up flutes on the bit. The bit assembly has chambers to hold the powder until it can be transferred to the sample-handling mechanisms of the rover's Collection and Handling for In-Situ Martian Rock Analysis (CHIMRA) device.

Before the rock powder is analyzed, some will be used to scour traces of material that may have been deposited onto the hardware while the rover was still on Earth, despite thorough cleaning before launch.

"We'll take the powder we acquired and swish it around to scrub the internal surfaces of the drill bit assembly," said JPL's Scott McCloskey, drill systems engineer. "Then we'll use the arm to transfer the powder out of the drill into the scoop, which will be our first chance to see the acquired sample."


Image above: NASA's Mars rover Curiosity used its Mast Camera (Mastcam) to take the images combined into this mosaic of the drill area, called "John Klein." Image credit: NASA/JPL-Caltech/MSSS.

 "Building a tool to interact forcefully with unpredictable rocks on Mars required an ambitious development and testing program," said JPL's Louise Jandura, chief engineer for Curiosity's sample system. "To get to the point of making this hole in a rock on Mars, we made eight drills and bored more than 1,200 holes in 20 types of rock on Earth."

Inside the sample-handling device, the powder will be vibrated once or twice over a sieve that screens out any particles larger than six-thousandths of an inch (150 microns) across. Small portions of the sieved sample will fall through ports on the rover deck into the Chemistry and Mineralogy (CheMin) instrument and the Sample Analysis at Mars (SAM) instrument. These instruments then will begin the much-anticipated detailed analysis.

Simulation of Martian Bedrock Drilling

The rock Curiosity drilled is called "John Klein" in memory of a Mars Science Laboratory deputy project manager who died in 2011. Drilling for a sample is the last new activity for NASA's Mars Science Laboratory Project, which is using the car-size Curiosity rover to investigate whether an area within Mars' Gale Crater has ever offered an environment favorable for life.

JPL manages the project for NASA's Science Mission Directorate in Washington.

For images and more information about the mission, visit: http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl/ .

You can follow the mission on Facebook and Twitter at: http://www.facebook.com/marscuriosity and http://www.twitter.com/marscuriosity

Image (mentioned), Video, Text, Credits: NASA / Dwayne Brown / JPL / Guy Webster.

Greetings, Orbiter.ch

NASA's Successful Robotic Refueling Demo Points To a Bright Satellite - Servicing Future












ISS - International Space Station patch.

Feb. 09, 2013

Following six historic days of operations aboard the International Space Station, NASA's Robotic Refueling Mission, or RRM, demonstrated remotely controlled robots using current-day technology could refuel satellites not designed to be serviced.

RRM tests from January 14-25 culminated in a first-of-its-kind robotic fluid transfer, a demonstration that could be a catalyst to expanded robotic satellite-servicing capabilities and lead to a greener, more sustainable space. NASA also hopes that RRM technologies may help boost the commercial satellite-servicing industry.


Image above: The Robotic Refueling Mission, or RRM, investigation (center, on platform) uses the International Space Station's Canadarm2 and the Canadian Dextre robot (right) to demonstrate satellite-servicing tasks. (NASA).

"RRM gives NASA and the emerging commercial satellite servicing industry the confidence to robotically refuel, repair and maintain satellites in both near and distant orbits -- well beyond the reach of where humans can go today," said Frank Cepollina, associate director of the Satellite Servicing Capabilities Office, or SSCO at NASA's Goddard Space Flight Center in Greenbelt, Md.

New Technologies for a New Industry

Since 2009, SSCO has aggressively advanced robotic technologies for a notional, free-flying, servicer spacecraft that could access, repair and refuel satellites in geosynchronous Earth orbit, or GEO. RRM is a critical part of this technology development campaign.

"RRM allows us to take a major step into the future -- a future where humans and machines can together take on greatly expanded roles in space capability, research and exploration," Cepollina said.


Image above: Stray drops of ethanol remain on the RRM Nozzle Tool after it withdraws from the fuel valve and the newly attached "quick disconnect" fitting. (NASA).

Veterans of five manned servicing missions to NASA's Hubble Space Telescope, Cepollina and the SSCO team conceived the idea of RRM and saw it through its rapid 18-month development to its July 2011 launch on STS-135, the last space shuttle mission. A joint effort with the Canadian Space Agency, RRM uses the space station as test bed for the research and development of robotic satellite-servicing capabilities.

The cutting-edge technologies RRM demonstrates could extend the lives of many of the hundreds of satellites currently in GEO. These assets deliver such essential services as weather reports, cell phone communications, television broadcasts, government communications and air traffic management.


Image above: Stephen Roderick supports an autonomous rendezvous and capture test in Goddard's Satellite Servicing Center, an incubator for cutting-edge satellite-servicing technologies. (NASA).

Servicing capabilities could greatly expand options for government and commercial fleet operators in the future, potentially delivering stakeholders significant savings in spacecraft replacement and launch costs.

RRM: A First-of-Its-Kind Refueling

The January RRM activities employed the teleoperated Canadian Dextre robot, four sophisticated RRM tools and the washing-machine-sized RRM module to execute an end-to-end refueling demonstration on orbit. Unlike other demos, RRM is the first to test the robotic refueling of satellite interfaces not designed to be accessed or serviced.


This artist's concept shows a servicing spacecraft, left, approaching a client satellite. NASA is developing technology needed to bring a high-technology "gas pump, robotic mechanic and tow truck" to satellites in orbit. (NASA).

Robot controllers at NASA's Johnson Space Center in Houston first commanded an RRM tool -- working at the end of more than 70 feet (21.34 meters) of combined Dextre and Canadarm2 robotics -- to cut a pair of twisted wires each 0.02 inches in diameter, the thickness of four sheets of paper. Additional exacting tasks followed, with RRM tools cutting more wire -- used to secure satellite parts during launch -- and unscrewing and stowing two protective caps before finally exposing the representative fuel valve.

After the Johnson team threaded the RRM Nozzle tool with its attached hose onto the valve, operators at NASA's Marshall Space Flight Center in Huntsville, Ala., sent a precise sequence of commands to activate the RRM Fluid Transfer System. Liquid ethanol flowed from the Fluid Transfer System into the Nozzle Tool and through the attached fuel valve, ultimately pulsing back into the module's reservoir. Once the fluid transfer was complete, the Nozzle Tool used a novel technique to withdraw from the valve, leaving behind a clever "quick disconnect" fitting that would allow for a simpler and more efficient future refueling connection.

Future RRM tasks scheduled for 2013 include thermal blanket cutting, and fastener and electronic termination cap removals: all firsts of their kinds. A new round of servicing task boards, tools and activities are slated to continue its investigations through 2015.

RRM: Mission to the Future Delivers

Results Straight from Space

Results of RRM operations show that current-day robotic technology can refuel the common, triple-sealed satellite fuel valves of orbiting satellites. "The RRM tools, technologies and techniques passed their tests with flying colors," said SSCO deputy project manager Benjamin Reed. "We are immensely pleased with its success and very grateful to our partner the Canadian Space Agency."

The team's excitement in completing the task was heightened by the treasury of experience and insight gained from the exercise.

"Nothing compares to seeing how your hardware and procedures work in a real space environment," said Reed. "This is the beauty of being able to test new, game-changing technologies on the International Space Station."

"We were very excited to see the RRM refueling task validated the ground development work that our dedicated SSCO team performs every day," Reed said. "It is direct evidence that we are not working blindly in the proverbial vacuum, but rather that our carefully planned work at Goddard accurately simulates the real environment of space."

SSCO plans to present RRM results to date at the upcoming Satellite 2013 conference, as well as during space station panels and other events.

What's Next?

NASA continues to test capabilities for a new robotic servicing frontier. In conjunction with RRM, the SSCO team has been studying a conceptual servicing mission and building technologies to address uncharted territory. They include an autonomous rendezvous and capture system, a propellant transfer system for zero gravity and specialized algorithms to orchestrate and synchronize satellite-servicing operations.

On Jan. 15, NASA released a Request for Information to seek input on a potential public-private partnership to effect the full utilization of NASA-developed technology through an end-to-end technology demonstration of a satellite-servicing capability for client satellites located in GEO. The conceptual Restore Mission would potentially perform servicing operations in orbit in the 2018-2023 timeframe. RRM is proving the technology to achieve such a future mission.

"RRM is a harbinger of the next era in satellite fleet operations," Reed said. "It disrupts the accepted paradigm that a GEO satellite must be decommissioned at the end of its propellant reserves. Nearly 50 years of common practice is challenged with the options that RRM proves and foreshadows."

For information, updates and videos about RRM and NASA's satellite servicing activities, visit: http://ssco.gsfc.nasa.gov

For more information about the International Space Station and its crew, visit:
http://www.nasa.gov/station

Related links:

Canadian Space Agency (CSA-ASC): http://www.asc-csa.gc.ca/eng/default.asp

Satellite Servicing Capabilities Office (SSCO): http://ssco.gsfc.nasa.gov/index.html

Robotic Refueling Mission (RRM): http://ssco.gsfc.nasa.gov/rrm_refueling_task.html

Images (mentioned), Video, Text, Credit: NASA's Goddard Space Flight Center / Adrienne Alessandro.

Best regards; Orbiter.ch

vendredi 8 février 2013

Is the ozone layer on the road to recovery??








ESA - MetOp weather satellite logo.

8 February 2013

 Antarctic ozone hole 2011 and 2012

Satellites show that the recent ozone hole over Antarctica was the smallest seen in the past decade. Long-term observations also reveal that Earth’s ozone has been strengthening following international agreements to protect this vital layer of the atmosphere.

According to the ozone sensor on Europe’s MetOp weather satellite, the hole over Antarctica in 2012 was the smallest in the last 10 years.

The instrument continues the long-term monitoring of atmospheric ozone started by its predecessors on the ERS-2 and Envisat satellites.

Since the beginning of the 1980s, an ozone hole has developed over Antarctica during the southern spring – September to November – resulting in a decrease in ozone concentration of up to 70%.

South Pole ozone

Ozone depletion is more extreme in Antarctica than at the North Pole because high wind speeds cause a fast-rotating vortex of cold air, leading to extremely low temperatures. Under these conditions, human-made chlorofluorocarbons – CFCs – have a stronger effect on the ozone, depleting it and creating the infamous hole.

Over the Arctic, the effect is far less pronounced because the northern hemisphere’s irregular landmasses and mountains normally prevent the build-up of strong circumpolar winds.

Reduced ozone over the southern hemisphere means that people living there are more exposed to cancer-causing ultraviolet radiation.

International agreements on protecting the ozone layer – particularly the Montreal Protocol – have stopped the increase of CFC concentrations, and a drastic fall has been observed since the mid-1990s.

However, the long lifetimes of CFCs in the atmosphere mean it may take until the middle of this century for the stratosphere’s chlorine content to go back to values like those of the 1960s.

The evolution of the ozone layer is affected by the interplay between atmospheric chemistry and dynamics like wind and temperature.

If weather and atmospheric conditions show unusual behaviour, it can result in extreme ozone conditions – such as the record low observed in spring 2011 in the Arctic – or last year’s unusually small Antarctic ozone hole.

Total ozone

To understand these complex processes better, scientists rely on a long time series of data derived from observations and on results from numerical simulations based on complex atmospheric models.

Although ozone has been observed over several decades with multiple instruments, combining the existing observations from many different sensors to produce consistent and homogeneous data suitable for scientific analysis is a difficult task.

Within the ESA Climate Change Initiative, harmonised ozone climate data records are generated to document the variability of ozone changes better at different scales in space and time.

With this information, scientists can better estimate the timing of the ozone layer recovery, and in particular the closure of the ozone hole.

MetOp weather satellite

Chemistry climate models show that the ozone layer may be building up, and the hole over Antarctica will close in the next decades.

Related links:

ESA's CCI ozone project: http://www.esa-ozone-cci.org/

BIRA/IASB: http://www.aeronomie.be/

KNMI: http://www.knmi.nl/index_en.html

DLR: http://www.dlr.de/dlr/en/desktopdefault.aspx/tabid-10002/

RT Solutions Inc.: http://www.rtslidort.com/

WMO ozone bulletin: http://www.wmo.int/pages/prog/arep/gaw/ozone/index.html

Graphics, Video, Text, Credits:  ESA / DLR / Eumetsat / NASA / WMO / GAW / KNMI / BIRA / IASB.

Cheers, Orbiter.ch

Hubble captures strobe flashes from a young star












ESA - Hubble Space Telescope logo.

Feb. 8, 2013

 Hubble image of LRLL 54361 and its surroundings

The NASA/ESA Hubble Space Telescope has produced a time-lapse movie of a mysterious protostar that behaves like a flashing light. Every 25.34 days, the object, designated LRLL 54361, unleashes a burst of light which propagates through the surrounding dust and gas. This is only the third time this phenomenon has been observed, and it is the most powerful such beacon seen to date. It is also the first to be seen associated with a light echo.

Hubble image of LRLL 54361

The cause of the fireworks seen in this Hubble image and video is hidden behind a dense disc and envelope of dust. However, astronomers think that the strobe effect is due to periodic interactions between two newly-formed stars that are gravitationally bound to each other.

These two stars drag material inwards from a surrounding disc of gas and dust. Astronomers propose that the light flashes seen in this video are due to this material suddenly being dumped onto the growing stars as they near one another in their orbits, unleashing a blast of radiation.

Light echo around LRLL 54361

“The protostar has such large brightness variations with a precise period that it is very difficult to explain,” says James Muzerolle of the Space Telescope Science Institute in Baltimore, USA, who has recently studied this fascinating object using Hubble and NASA’s Spitzer Space Telescope. Spitzer made repeated observations over seven years, before Hubble was pointed towards the object to make detailed observations over the period of one pulse event.

How LRLL 54361 flashes like a strobe light

The Hubble observations uncover a spectacular movement of light away from the centre of the system, an optical illusion known as a light echo. While it might look like eruptions of gas are coming out of the protostar, these pulses are actually flashes of light propagating through the surrounding dust and gas and reflecting towards the observer: there is no substantial physical motion within the cloud over these timescales.

Light echoes from LRLL 54361 (non-annotated)

Flashing double star systems like this one are rare, because close binaries account for only a few percent of our galaxy’s stellar population. Moreover, the pulsing light is likely to be a brief phenomenon in the early life of a star.

Light echoes from LRLL 54361 (annotated)

Notes:

The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

Links:

Images of Hubble: http://www.spacetelescope.org/images/archive/category/spacecraft/

A press release from NASA, with more information about scientific research into LRLL 54361 is available here: http://hubblesite.org/news/2013/04

Images, Videos, Text,  Credit: NASA, ESA, J. Muzerolle (STScI) / E. Furlan (NOAO, Caltech), and R. Hurt (Caltech).

Greetings, Orbiter.ch

jeudi 7 février 2013

Arianespace orbits Amazonas-3 and Azerspace / Africasat-1a satellites


















ARIANESPACE / ESA - Flight VA-212 poster.


Feb. 7, 2013

Arianespace orbits Amazonas-3 and Azerspace/Africasat-1a satellites; First Ariane 5 ECA mission in 2013 a success

Ariane 5 ECA Flight VA212 lift-off

Thursday, February 7, 2013,  the launch occurred at 21:36 GMT (4:36 p.m. EST) Arianespace successfully carried out the 54th Ariane 5 launch in a row, orbiting two telecommunications satellites: Amazonas-3 for Spanish operator Hispasat, and Azerspace/Africasat-1a for the Azerbaijani operator Azercosmos 0JSC and the Azerbaijan Ministry of Communications and Information Technologies.

Launch of first 2013 Ariane 5 with Amazonas-3 / Azerspace-1

First Ariane 5 launch of 2013 and a new record

Today's successful mission, the 54th in a row for the European launcher, once again proves the reliability and availability of the Ariane 5 launch system. It also confirms that Arianespace continues to set the standard for independent access to space for all operators, including national and international space agencies, private industry and governments.

The 68th launch of Ariane 5 set a new record for weight injected into geostationary transfer orbit: the launcher on this mission carried a total payload of 10,317 kg, including 9,503 kg for the two satellites, Amazonas-3 and Azerspace/Africasat-1a.

This was the first Ariane 5 launch in 2013. Its success once again illustrated the operational capability of this launcher, the only one now on the market capable of simultaneously launching two payloads.

Processing Highlights of the Ariane 5, Amazonas-3 / Azerspace

Launching satellites for a long-standing customer and a new operator
Arianespace provides the launch services most clearly matches the requirements of all operators.

Amazonas-3 is the seventh Spanish satellite launched by Arianespace. The company first launched the Hispasat 1A and 1B satellites in 1992 and 1993, respectively, followed in 2005 and 2006 by the XTAR-Eur and Spainsat satellites for Hispasat and its subsidiary Hisdesat. Amazonas-2 was launched in 2009, followed by Hispasat 1E in 2010.

The Azerspace/Africasat-1a satellite is the first national satellite to be launched by Arianespace for the Azerbaijan Ministry of Communications and Information Technologies.

Azerspace/Africasat-1a satellite separation from Ariane 5 second stage

Arianespace has already launched the first satellites for 31 operators to date. 

Amazonas-3 – Azerspace/Africasat-1a mission at a glance

The mission was carried out by an Ariane 5 ECA launcher from Europe's Spaceport in Kourou, French Guiana. Liftoff was on Thursday, February 7, 2013 at 6:36 pm local time in Kourou (4:36 pm in Washington, D.C., 21:36 UT, 10:36 pm in Paris, and 1:36 am on Friday, February 8 in Baku).

Amazonas-3 was built by Space Systems/Loral using the SSL 1300 platform and  weighed 6,265 kg at launch. It has 33 Ku-band transponders, 19 C-band transponders, and 9 Ka-band spot beams. This high-power satellite provides a wide range of telecommunications and broadband connectivity services in Europe, the Americas and North Africa. It offers a design life of 15 years. Amazonas-3 is the 43rd satellite built by Space Systems/Loral to be launched by Arianespace.

Amazonas-3 separation from Ariane 5 second stage

The Azerspace/Africasat-1a satellite was built by Orbital Sciences Corporation using a Star-2 platform. Weighing 3,000 kg at launch, the satellite is equipped with 24 C-band transponders and 12 Ku-band transponders. It will provide a wide range of telecommunications services for Azerbaijan, Central Asia, Europe, the Middle East and Africa.

Amazonas-3 satellite

Azerspace/Africasat-1a is the 24th satellite built by Orbital Sciences Corporation to be launched by Arianespace.

 Azerspace/Africasat-1a satellite

For more information about Arianespace, visit: http://www.arianespace.com/index/index.asp

Images, Text, Videos, Credits: ARIANESPACE / ARIANESPA TV / Space Systems / Loral / Orbital Sciences Corporation / Orbiter.ch Aerospace.

Best regards, Orbiter.ch