jeudi 1 février 2018

ROSCOSMOS: Soyuz-2.1А LV with two KANOPUS-V satellites lift off from Vostochny












ROSCOSMOS logo.

February 1, 2018

Soyuz-2.1А LV with two KANOPUS-V satellites lift off

On February 1, 2018 at 05:07:18 Moscow time, Soyuz-2.1a launch vehicle successfully lifted off from VOSTOCHNY Cosmodrome. The launch mission is to deliver 2 Earth observation Kanopus-V satellites (№3 and №4) and 9 smallsats piggybacked under the federal and commercial contracts of Glavkosmos to their target orbits.

According the flight program, the first three stages of Soyuz-2.1b have taken the ascent unit into low orbit just short of eight minutes and forty-eight seconds after liftoff. From this point in the mission, the Fregat upper stage performs planned mission maneuvers to advance the satellites to their planned orbits. Separation of the Kanopus-V satellites is scheduled to occur approximately 1 hour after lift-off.

Launch of the Soyuz-2-1a carrying the Canopus-V spacecraft 3 and 4

Soyuz-2 launcher is based on the Soyuz-U series. Soyuz-2 features advanced engines and up-to-date control and telemetry systems that significantly enhance the LV technical and operational specifications. The upgrading was done in two phases. At phase 1а, a standardized Soyuz-2.1a was born to accommodate various upper composites with fairings of up to 4.11m in diameter. The LV is capable to orbit a payload with improved accuracy; the upgraded control system and stage I-II engines have allowed for increasing of the payload mass to be lofted to the low Earth orbit. At phase 1b resulted in Soyuz-2.1b, stage III was refitted with a state-of-the-art 14D23 (RD-0124) engine which made its performance even better.

Kanopus-V satellite

The prime LV designer is Progress Space Rocket Center (the city of Samara). Depending on a mission, Soyuz-2 launcher can be configured with the Fregat upper stage. A standard Fregat upper stage was designed by Lavochkin Association to complement various launchers in order to put satellites in different orbits. It is used in Soyuz rockets. A standard Fregat upper stage equipped with extra fuel tanks or drop-off tanks evolved to highly efficient upper stage modifications: Fregat-MT and Fregat-SB.

Roscosmos Press Release: http://en.roscosmos.ru/20712/

Images, Video Text, Credits: Roscosmos/Günter Space Page.

Greetings, Orbiter.ch

Mount Sharp 'Photobombs' Mars Curiosity Rover












NASA - Mars Science Laboratory (MSL) patch.

February 1, 2018


Image above: This self-portrait of NASA's Curiosity Mars rover shows the vehicle on Vera Rubin Ridge, which it's been investigating for the past several months. Poking up just behind Curiosity's mast is Mount Sharp, photobombing the robot's selfie. Image credits: NASA/JPL-Caltech/MSSS.

A new self-portrait of NASA's Curiosity Mars rover shows the vehicle on Vera Rubin Ridge, which it has been investigating for the past several months. Directly behind the rover is the start of a clay-rich slope scientists are eager to begin exploring. In coming weeks, Curiosity will begin to climb this slope. In the image, north is on the left and west is on the right, with Gale Crater's rim on the horizon of both edges.

Poking up just behind Curiosity's mast is Mount Sharp, photobombing the robot's selfie. When Curiosity landed on Mars five years ago, the team's intention was to study lower Mount Sharp, where the rover will remain for all of its time on Mars. The mountain's base provides access to layers formed over millions of years. These layers formed in the presence of water -- likely due to a lake or lakes where sediments accumulated, which formed these layers inside Gale Crater.

The mosaic was assembled from dozens of images taken by Curiosity's Mars Hands Lens Imager (MAHLI). They were all taken on Jan. 23, 2018, during Sol 1943.

For news about other Mars missions this month, view the first episode of a new video series, "The Mars Report."

NASA Mars Report January 31, 2018

Video above: In this first episode of The Mars Report we celebrate the 14th anniversary of the Opportunity rover; show you a recent panoramic view from the Curiosity rover; and recap a "cool" discovery of ice deposits spotted by the Mars Reconnaissance Orbiter. Also, we look forward to the InSight lander, heading to the Red Planet in May 2018. Video Credits: NASA Jet Propulsion Laboratory.

Additional information about NASA's exploration of Mars is at: https://mars.nasa.gov/

Mars Science Laboratory (Curiosity): https://www.nasa.gov/mission_pages/msl/index.html

Image (mentioned), Video (mentioned), Text, Credits: NASA/JPL/Andrew Good.

Greetings, Orbiter.ch

mercredi 31 janvier 2018

SpaceX - GovSat-1 Mission Success












SpaceX - GovSat-1 Mission patch.

Jan. 31, 2018

GovSat-1 Successfully Launched on SpaceX Falcon 9 Rocket

On Wednesday, January 31st, SpaceX successfully launched the GovSat-1 satellite to a Geostationary Transfer Orbit (GTO) from Space Launch Complex 40 (SLC-40) at Cape Canaveral Air Force Station, Florida.

GovSat-1 Launch

The satellite was deployed approximately 32 minutes after launch, putting the GovSat-1 satellite into its targeted orbit.

Falcon 9’s first stage for the GovSat-1 mission previously supported the NROL-76 mission from LC-39A in May 2017.

GovSat-1 communications satellite

GovSat 1 communications satellite for LuxGovSat, a joint venture between SES and the government of Luxembourg. The GovSat 1 satellite, also known as SES 16, will provide secure military X-band and Ka-band communications links, helping support Luxembourg’s NATO obligations. The satellite was built by Orbital ATK.

For more information about SpaceX, visit: http://www.spacex.com/

Images, Video, Text, Credits: SpaceX/SES/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch

SPHERES Science and Vision Checks Ahead of Friday Spacewalk & Full Moon









ISS - Expedition 54 Mission patch.

January 31, 2018


Image above: Full Moon seen by Griffith Observatory and EarthCam channel on ISS, speed: 27'567 Km/h, altitude: 419,95 Km, image captured by Roland Berga (on Earth in Switzerland) from International Space Station (ISS) using ISS-HD Live application with EarthCam's from ISS on January 31, 2018 at 14:53 UTC.

As the International Space Program gets ready for a pair of spacewalks in February, the Expedition 54 crew was busy setting up a pair of experimental internal satellites and conducting vision checks today.

NASA astronauts Joe Acaba and Mark Vande Hei brought out a pair of tiny satellites, also known as SPHERES (Synchronized Position Hold, Engage, Reorient, Experimental Satellites), for a run of the SmoothNAV experiment today. The study is researching how algorithms and sensors may help determine relative positions and velocities between spacecraft.

Both astronauts also joined Flight Engineers Scott Tingle and Norishige Kanai for eye exams during the afternoon. Tingle and Kanai first swapped roles as Crew Medical Officer checking each other’s eyes today using optical coherence tomography. Then Tingle joined Acaba and Vande Hei afterward for more eye checks using a fundoscope. Doctors on the ground remotely assisted the astronauts viewing their eyes in real time.


Image above: A pair of empty Russian Orlan spacesuits are pictured inside the airlock of the Pirs docking compartment. The spacesuits will be worn during a Feb. 2 spacewalk with cosmonauts Alexander Misurkin and Anton Shkaplerov. Image Credit: NASA.

Cosmonauts Alexander Misurkin and Anton Shkaplerov donned their Orlan spacesuits today to ensure a good fit and check for pressure leaks ahead of a spacewalk scheduled to start Friday at 10:30 a.m. EST. They’ll work outside for about 6.5 hours of maintenance on the Russian side of the orbital laboratory.

The second spacewalk is set to take place Feb. 15 at 7:10 a.m. when Vande Hei and Kanai exit the station to continue robotics maintenance on the Canadarm2. They’ll stow a pair of latching end effectors, or robotic hands, which had been detached from the Canadarm2 on two previous spacewalks, the first on Oct. 5, 2017 and the second on Jan. 23.

International Space Station Transits the Full Moon


The International Space Station, with a crew of six onboard, is seen in silhouette as it transits the moon at roughly five miles per second on Tuesday, Jan. 30, 2018, from Alexandria, Va. Onboard are NASA astronauts Joe Acaba, Mark Vande Hei, and Scott Tingle; Russian Cosmonauts Alexander Misurkin and Anton Shkaplerov, and Japanese astronaut Norishige Kanai. Image Credits: NASA/Bill Ingalls.

Related links:

NASA TV: https://www.nasa.gov/multimedia/nasatv/index.html

Expedition 54: https://www.nasa.gov/mission_pages/station/expeditions/expedition54/index.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

Images (mentioned), Text, Credits: NASA/Mark Garcia/Brian Dunbar.

Best regards, Orbiter.ch

Glory From Gloom












ESO - European Southern Observatory logo.

31 January 2018

Star formation region Lupus 3

A dark cloud of cosmic dust snakes across this spectacular wide field image, illuminated by the brilliant light of new stars. This dense cloud is a star-forming region called Lupus 3, where dazzlingly hot stars are born from collapsing masses of gas and dust. This image was created from images taken using the VLT Survey Telescope and the MPG/ESO 2.2-metre telescope and is the most detailed image taken so far of this region.

The Lupus 3 dark cloud in the constellation of Scorpius

The Lupus 3 star forming region lies within the constellation of Scorpius (The Scorpion), only 600 light-years away from Earth. It is part of a larger complex called the Lupus Clouds, which takes its name from the adjacent constellation of Lupus (The Wolf). The clouds resemble smoke billowing across a background of millions of stars, but in fact these clouds are a dark nebula.

Wide-field view of the Lupus 3 dark cloud and associated hot young stars

Nebulae are great swathes of gas and dust strung out between the stars, sometimes stretching out over hundreds of light-years. While many nebulae are spectacularly illuminated by the intense radiation of hot stars, dark nebulae shroud the light of the celestial objects within them. They are also known as absorption nebulae, because they are made up of cold, dense particles of dust that absorb and scatter light as it passes through the cloud.

Famous dark nebulae include the Coalsack Nebula and the Great Rift, which are large enough to be seen with the naked eye, starkly black against the brilliance of the Milky Way.

Zooming in on the Lupus 3 star-forming region

Lupus 3 has an irregular form, appearing like a misshapen snake across the sky. In this image it is a region of contrasts, with thick dark trails set against the glare of bright blue stars at the centre. Like most dark nebulae, Lupus 3 is an active star formation region, primarily composed of protostars and very young stars. Nearby disturbances can cause denser clumps of the nebula to contract under gravity, becoming hot and pressurised in the process. Eventually, a protostar is born out of the extreme conditions in the core of this collapsing cloud.

The two brilliant stars in the centre of this image underwent this very process. Early in their lives, the radiation they emitted was largely blocked by the thick veil of their host nebula, visible only to telescopes at infrared and radio wavelengths. But as they grew hotter and brighter, their intense radiation and strong stellar winds swept the surrounding areas clear of gas and dust, allowing them to emerge gloriously from their gloomy nursery to shine brightly.

Panning across the Lupus 3 star-forming region

Understanding nebulae is critical for understanding the processes of star formation — indeed, it is thought that the Sun formed in a star formation region very similar to Lupus 3 over four billion years ago. As one of the closest stellar nurseries, Lupus 3 has been the subject of many studies; in 2013, the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile captured a smaller picture of its dark smoke-like columns and brilliant stars (eso1303).

More information:

ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory by far. It is supported by 16 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile and by Australia as a strategic partner. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world’s most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world’s largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is a major partner in ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre Extremely Large Telescope, the ELT, which will become “the world’s biggest eye on the sky”.

Related links:

eso1303: http://www.eso.org/public/news/eso1303/

ESOcast 148 Light: Clouded Star Birth: https://www.eso.org/public/videos/eso1804b/

ESO’s La Silla Observatory: https://www.eso.org/public/teles-instr/lasilla/

MPG/ESO 2.2-metre telescope: https://www.eso.org/public/teles-instr/lasilla/mpg22/

Research review paper: https://www.eso.org/public/archives/releases/sciencepapers/eso1303/eso1303a.pdf

Photos of the VLT Survey Telescope: https://www.eso.org/public/images/archive/search/?adv=&subject_name=VLT%20Survey%20Telescope

Photos of the MPG/ESO 2.2-metre telescope: https://www.eso.org/public/images/archive/search/?adv=&subject_name=mpg

Images, Text, Credits: ESO/Richard Hook/R. Colombari/IAU and Sky & Telescope/Digitized Sky Survey 2/ Acknowledgement: Davide De Martin/Videos: ESO/R. Colombari/Digitized Sky Survey 2/N. Risinger (skysurvey.org). Music: Astral electronic.

Greetings, Orbiter.ch

mardi 30 janvier 2018

Rescheduled Robotics Work Makes Two Spacewalks in February









ISS - Expedition 54 Mission patch.

Jan. 30, 2018

Saying Goodnight

Image above: "Good night from @Space_Station. DC, NY, Toronto, Cleveland, and surrounding areas!" This note from NASA astronaut Mark Vande Hei may be visually stunning, but it's a common occurrence on the International Space Station, which experiences 16 sunrises and sunsets every day. Image Credits: NASA/Mark Vande Hei.

International Space Station managers have rescheduled a U.S. spacewalk postponed on Monday to mid-February. Meanwhile, the Expedition 54 crew is also preparing for a Russian spacewalk this Friday.

Astronauts Mark Vande Hei and Norishige Kanai are planning to begin their spacewalk Feb. 15 at 7:10 a.m. EST to stow and reposition a pair of Latching End Effectors (LEEs). The LEEs are robotic hands attached to the tip of the Canadarm2 that grapple and release cargo ships and external station hardware.

During the 6.5-hour excursion, the spacewalkers will first move an older LEE from a bracket on the Mobile Base System on the truss to the Quest airlock. It was removed from Canadarm2 during a spacewalk last October. Next, a degraded LEE detached from Canadarm2 during the last U.S. spacewalk on Jan. 23 will be moved from an external stowage platform to the Mobile Base System. NASA TV will begin its live broadcast of the spacewalk at 5:30 a.m.


Image above: Astronaut Scott Tingle works on a U.S. spacesuit inside the Quest airlock at the beginning of January 2018 before a pair of robotics maintenance spacewalks were scheduled to begin. Image Credit: NASA.

Cosmonauts Alexander Misurkin and Anton Shkaplerov will exit the Pirs airlock in their Orlan spacesuits Friday at around 10:30 a.m. for 6.5 hours of Russian maintenance, highlighted by the swap out of an electronics system for the Zvezda Service Module’s high gain communications antenna. Live NASA TV coverage begins at 9:45 a.m.

Earlier today, Zvezda’s engines fired for 23 seconds to increase the station’s altitude and set up operations for the arrival of cargo and the departure of crew. The Progress 69 cargo craft will launch from the Baikonur Cosmodrome in Kazakhstan Feb. 11, then 3 Expedition 54 crew members will depart the station in their Soyuz MS-06 spacecraft Feb. 27 for a landing in Kazakhstan later that day.

Related links:

NASA TV: https://www.nasa.gov/multimedia/nasatv/index.html

Expedition 54: https://www.nasa.gov/mission_pages/station/expeditions/expedition54/index.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

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

Best regards, Orbiter.ch

NASA’s Small Spacecraft Produces First 883-Gigahertz Global Ice-Cloud Map












NASA Goddard Space Flight Center logo.

Jan. 30, 2018

A bread loaf-sized satellite has produced the world’s first map of the global distribution of atmospheric ice in the 883-Gigahertz band, an important frequency in the submillimeter wavelength for studying cloud ice and its effect on Earth’s climate.

IceCube — the diminutive spacecraft that deployed from the International Space Station in May 2017— has demonstrated-in-space a commercial 883-Gigahertz radiometer developed by Virginia Diodes Inc., or VDI, of Charlottesville, Virginia, under a NASA Small Business Innovative Research contract. It is capable of measuring critical atmospheric cloud ice properties at altitudes between 3-9 miles (5 Km-15 Km).


Image above: The bread loaf-sized IceCube was deployed from the International Space Station in May. One month later, it began science operations gathering global data about atmospheric ice clouds in the submillimeter wavelengths. Image Credit: NASA.

NASA scientists pioneered the use of submillimeter wavelength bands, which fall between the microwave and infrared on the electromagnetic spectrum, to sense ice clouds. However, until IceCube, these instruments had flown only aboard high-altitude research aircraft. This meant scientists could gather data only in areas over which the aircraft flew.

“With IceCube, scientists now have a working submillimeter radiometer system in space at a commercial price,” said Dong Wu, a scientist and IceCube principal investigator at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “More importantly, it provides a global view on Earth’s cloud-ice distribution.”

Sensing atmospheric cloud ice requires scientists deploy instruments tuned to a broad range of frequency bands. However, it’s particularly important to fly submillimeter sensors. This wavelength fills a significant data gap in the middle and upper troposphere where ice clouds are often too opaque for infrared and visible sensors to penetrate. It also reveals data about the tiniest ice particles that can’t be detected clearly in other microwave bands.

The Technical Challenge

IceCube’s map is a first of its kind and bodes well for future space-based observations of global ice clouds using submillimeter-wave technology, said Wu, whose team built the spacecraft using funding from NASA’s Earth Science Technology Office’s (ESTO) In-Space Validation of Earth Science Technologies (InVEST) program and NASA’s Science Mission Directorate CubeSat Initiative. The team’s challenge was making sure the commercial receiver was sensitive enough to detect and measure atmospheric cloud ice using as little power as possible.


Image above: IceCube Principal Investigator Dong Wu set out to demonstrate a commercial 883-Gigahertz radiometer in space, but ended up getting much more: the world’s first ice-cloud map in that frequency. Here he is pictured holding the instrument. Image Credit: NASA.

Ultimately, the agency wants to infuse this type of receiver into an ice-cloud imaging radiometer for NASA’s proposed Aerosol-Cloud-Ecosystems, or ACE, mission. Recommended by the National Research Council, ACE would assess on a daily basis the global distribution of ice clouds, which affect the Earth’s emission of infrared energy into space and its reflection and absorption of the Sun’s energy over broad areas. Before IceCube, this value was highly uncertain.

“It speaks volumes that our scientists are doing science with a mission that primarily was supposed to demonstrate technology,” said Jared Lucey, one of IceCube’s instrument engineers. He was one of only a handful of scientists and engineers at Goddard and NASA’s Wallops Flight Facility in Virginia who developed IceCube in just two years. “We met our mission goals and now everything else is bonus,” he said.

Multiple Lessons Learned

In addition to demonstrating submillimeter-wave observations from space, the team gained important insights into how to efficiently develop a CubeSat mission, determining which systems to make redundant and which tests to forgo because of limited funds and a short schedule, said Jaime Esper, IceCube’s mission systems designer and technical project manager at Goddard.


Image above: Relatively small teams from both Goddard and the Wallops Flight Facility built the IceCube mission. The Goddard team included (left photo, back row, from left to right): Dong Wu, Michael Solly, Jared Lucey, Jeffrey Piepmeier, Paul Racette, Derek Hudson; (front row, left to right): Melyane Ortiz-Acosta, Armi Pellerano, Carlos Duran-Aviles, Kevin Horgan, Negar Ehsan, and Mark Wong. Image Credit: NASA.

“It wasn’t an easy task,” said Negar Ehsan, IceCube’s instrument system lead. “It was a low-budget project” that required the team to develop both an engineering test unit and a flight model in a relatively short period of time. In spite of the challenges, the team delivered the VDI-provided instrument on time and budget. “We demonstrated for the first time 883-Gigahertz observations in space and proved that the VDI-provided system works appropriately,” she said. “It was rewarding.”

The team used commercial off-the-shelf components, including VDI’s radiometer. The components came from multiple commercial providers and didn’t always work together harmoniously, requiring engineering. The team not only integrated the radiometer to the spacecraft, but also built spacecraft ground-support systems and conducted thermal-vacuum, vibration, and antenna testing at Goddard and Wallops.

“IceCube isn’t perfect,” Wu conceded, referring to noise or slight errors in the radiometer’s data. “However, we can make a scientifically useful measurement. We came away with a lot of lessons learned from this CubeSat project, and next time engineers can build it much more quickly.”


Image above: The Wallops team included (right photo, back row, from left to right): Chris Purdy, Brian Abresch, Alex Coleman, and Kurt Reddersen; (front row, from left to right): Brooks Flaherty, Scott Heatwole, Jerry Cote, Henry Hart, Bob Stancil, and Ted Daisey. Image Credit: NASA.

“This is a different mission model for NASA,” Wu continued. “Our principal goal was to show this small mission could be done. The question was, could we can get useful science and advance space technology with a low-cost CubeSat developed under an effective government-commercial partnership. I believe the answer is yes.”

Small satellites, including CubeSats, are playing an increasingly larger role in exploration, technology demonstration, scientific research and educational investigations at NASA, including: planetary space exploration; Earth observations; fundamental Earth and space science; and developing precursor science instruments like cutting-edge laser communications, satellite-to-satellite communications and autonomous movement capabilities.

NASA ESTO supports InVEST missions like IceCube and technologies at NASA centers, industry and academia to develop, refine and demonstrate new methods for observing Earth from space, from information systems to new components and instruments.

For more Goddard technology news, go to https://www.nasa.gov/sites/default/files/atoms/files/winter_2018_final_lowrez.pdf

Related links:

NASA’s proposed Aerosol-Cloud-Ecosystems, or ACE: https://eospso.gsfc.nasa.gov/missions/aerosol-cloud-ecosystems

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

NASA ESTO: https://esto.nasa.gov/

Images (mentioned), Text, Credits: NASA/Lynn Jenner/Goddard Space Flight Center, by Lori Keesey.

Greetings, Orbiter.ch