jeudi 27 septembre 2018

Norway takes the lead in hybrid propulsion













NAMMO GROWTH WORX logo.

27 September 2018

Today, Norway’s first hybrid rocket to reach space demonstrated new hybrid propulsion technology for a cleaner, safer, more flexible method of powering small launch vehicles.

Soaring up to five times the speed of sound from the Andøya Space Center, the 9 m long Nucleus sounding rocket passed the edge of Earth’s atmosphere to reach an altitude of over 107 km in less than three minutes.

Nucleus lifts off

After its suborbital flight it returned to Earth, splashing down in the Atlantic Ocean, 180 km off the coast of Norway. Its payload, supplied by the Andøya Space Center, comprised electronics that transmitted inflight data and video for further analysis, as well as a dispenser to eject six ‘daughter payloads’ at altitude.

Nammo in partnership with ESA’s Future Launchers Preparatory Programme designed and built the new hybrid motor driving this rocket. The motor combines liquid and solid propellant.

Nammo chose highly concentrated liquid hydrogen peroxide as the oxidiser reacting with a rubber-like substance as fuel. These substances are safe to handle and the byproducts of combustion are mostly water and carbon dioxide – making the motor environmentally friendly too.

The oxidiser and solid fuel remain separated inside the rocket until mixed at ignition. Hybrid propellants have low evaporation rates so the rocket can be loaded safely, well before launch. This reduces the cost of launch service operations compared with other technologies.

The fuel being a non-toxic, non-explosive solid simplifies manufacturing and handling, further lowering cost.

Nucleus sounding rocket

Being able to vary the flow of oxidiser during flight and thus the thrust meets a wide range of mission requirements, the motor can even be shut down and reignited for complex missions.

The aim is for hybrid propulsion to match the precision offered through liquid propulsion, while lowering risks and costs, which would be ideal for smaller European launch sites like the Andøya Space Center.

Today’s demonstration will provide valuable data on the behaviour of this hybrid propulsion system in flight. The next step is to build a larger motor to increase thrust from today’s 30kN to about 75–100 kN, extend the burn time, and to reduce weight and cost.

"Hybrid technology has the potential to become a highly competitive building block for an orbital launcher – our ultimate goal,” commented Adrien Boiron, Chief engineer at Nammo.

Related links:

Future Launchers Preparatory Programme: http://www.esa.int/Our_Activities/Space_Transportation/New_Technologies/FLPP_preparing_for_Europe_s_next-generation_launcher

Andøya Space Center: https://www.andoyaspace.no/

Nammo: https://www.nammo.com/

Nammo explains technology behind Nucleus: https://www.youtube.com/watch?v=-Sug8Fdu_vU

Space Transportation: http://www.esa.int/Our_Activities/Space_Transportation

Images, Text, Credits: ESA/Nammo.

Greetings, Orbiter.ch

Hayabusa2 Touches Down Ryugu












JAXA - Hayabusa2 Mission patch.

September 27, 2018

JAXA operated Hayabusa2 to separate and send its onboard rovers MINERVA-II1 to the surface of the target asteroid Ryugu.

MINERVA-II1, the collective name of Rovers-1A and –B, have landed on Ryugu. Both rovers are in good health, commencing the survey of the asteroid's surface.

Following MINERVA-II1 deployment, the Hayabusa2 spacecraft returned to its home position altitude, approximately 20 kilometers above the center of the asteroid at 3 p.m. in Japan time, September 22, 2018. The status of Hayabusa2 is nominal as well.

Images photographed by MINERVA-II1 (Images credit: JAXA)


Image above: Image captured by Rover-1B on September 21 at around 13:07 JST. This color image was taken immediately after separation from the spacecraft. The surface of Ryugu is in the lower right. The coloured blur in the top left is due to the reflection of sunlight when the image was taken.


Image above: mage captured by Rover-1A on September 22 at around 11:44 JST. Color image captured while moving (during a hop) on the surface of Ryugu. The left-half of the image is the asteroid surface. The bright white region is due to sunlight.

On 21 September 2018, 180 million miles from Earth, a roughly 1.5 square-metre cube descended towards a primitive space rock. After years of planning and 4 years in flight, this tiny spacecraft captured this ‘shadow selfie’ as it closed in on asteroid Ryugu, just 80 metres from the remnant of our Solar System’s formation, 4.6 billion years ago.

The Hayabusa2 spacecraft is operated by the Japanese Space Agency (JAXA), supported in part by ESA's Estrack Malargüe deep-space tracking station. The spacecraft carries four small landers that will investigate the asteroid’s surface, all four designed to gently fall onto the surface of the rocky boulder, taking advantage of its low gravity environment.

Around the time this remarkable picture was taken, the spacecraft released its two MINERVA-II1 rovers which have since successfully landed and demonstrated an ability to hop around this rock-strewn body.

A shadowy selfie taken 180 million miles away

"I cannot find words to express how happy I am that we were able to realize mobile exploration on the surface of an asteroid" enthused Yuichi Tsuda, Hayabusa2 Project Project Manager, "I am proud that Hayabusa2 was able to contribute to the creation of this technology for a new method of space exploration by surface movement on small bodies."

The next stage will see the Mobile Asteroid Surface Scout (MASCOT) lander released onto the asteroid’s surface. Developed by the German Aerospace Center (DLR) in cooperation with the French Space Agency (CNES) MASCOT has enough power for a 12-hour mission, in which it will analyse the asteroid’s surface at two different sites.

The Hayabusa2 spacecraft itself will collect three samples from Ryugu, bringing them back to Earth in December 2020. These strange specimens will provide insights into the composition of this carbonaceous asteroid — a type of space rock expected to preserve some of the most pristine materials in the Solar System.


Image above: This artist's rendering depicts Japan's Hayabusa2 probe reaching the asteroid Ryugu, thought to contain organic matter from the dawn of the solar system. (Image courtesy of JAXA).

As well as hopefully shining light on the origin and evolution of the inner planets, and the sources of water and organic compounds on Earth, this knowledge should help in efforts to protect our planet from marauding masses that come too close for comfort to our home planet.

Understanding the composition and characteristics of near-Earth objects is vital to defending ourselves from them, if one were to head in our direction. ESA’s proposed Hera mission to test asteroid deflection is an ambitious example of how we can get to know these ancient bodies better, all in the name of planetary defence.

Related link:

JAXA website on Hayabusa2 Project: http://www.hayabusa2.jaxa.jp/en/

Asteroid Explorer "Hayabusa2": http://global.jaxa.jp/projects/sat/hayabusa2/index.html

Images (mentioned), Text, Credits: Japan Aerospace Exploration Agency (JAXA)/National Research and Development Agency/European Space Agency (ESA).

Greetings, Orbiter.ch

mercredi 26 septembre 2018

History of Airborne Astronomy at NASA














NASA - Armstrong Flight Research Center patch / NASA & DLR - SOFIA patch.

Sept. 26, 2018

Sixty years ago, in 1958, NASA was founded as the National Aeronautics and Space Administration. The agency has a long history of using airplanes to study space. Flying at high altitudes puts telescopes above the water vapor in Earth’s atmosphere that blocks certain types of light, like infrared, from reaching ground-based telescopes. Airborne observatories can also go anywhere to conduct observations, enabling researchers to study transient events, such as the eclipse-like events called occultations to learn about distant planets and objects. When airborne observatories land after each flight, the telescope instruments, such as specialized cameras, can be upgraded or serviced, and new ones can be built to harness new technologies — which is not possible on most space-based telescopes.


Image above: NASA’s Galileo I aircraft during a flight to study a solar eclipse in 1965. The modified Convair-990 aircraft had multiple observations windows in the top left side of the aircraft. Image Credit: NASA.  

NASA paved the way for airborne astronomy in 1965 by flying a modified Convair 990 aircraft to study a solar eclipse from inside the path of totality. In 1968, astronomers used 12-inch telescopes in the cabins of Learjet aircraft to study objects like Venus using infrared light.


Images above: Left: The Learjet Observatory (Learjet 24B aircraft) flying above California in the early 1970’s. The telescope was just in front of the wing. Right: Scientist Carl Gillespie using a 12-inch infrared telescope while flying aboard the Learjet 23 aircraft at 50,000 feet in 1968. Image Credit: NASA.

The work on the Learjet Observatory led to the development of NASA's Kuiper Airborne Observatory, or KAO, a converted C-141 cargo aircraft that carried a 36-inch reflecting telescope. Named after the planetary scientist Gerard Kuiper, it operated from NASA’s Ames Research Center in California from 1975 to 1995. Scientists used the KAO for solar system research, galactic and extra-galactic observations, and even studied the space shuttle’s heat shield in infrared light as it re-entered Earth’s atmosphere. Discoveries made from the Kuiper Airborne Observatory included:

- Pluto’s atmosphere
- Rings around Uranus
- ​A ring of star formation around the center of the Milky Way
- Complex organic molecules in space
- Water in comets and in Jupiter’s atmosphere


Images above: Left: The Kuiper Airborne Observatory flies with its telescope door open in 1980. The converted C-141 aircraft had a 36-inch telescope just in front of the wing. Right: Inside the KAO, where the mission crew sat during flight. These consoles were positioned along the side of the aircraft's cabin. The portion of the telescope system that was inside the cabin can be seen at the back of the image. The open telescope cavity was separate from the pressurized cabin. Image Credit: NASA.
The Kuiper Airborne Observatory was decommissioned in 1995 to enable the development of a flying observatory with a larger, more powerful infrared telescope — the Stratospheric Observatory for Infrared Astronomy (SOFIA).

NASA and the German Aerospace Center (DLR) jointly operate SOFIA. They chose a Boeing 747SP aircraft to carry the largest airborne telescope to date, at 106 inches (2.7 meters) in diameter. NASA modified and maintains the aircraft — which once flew for both Pan American World Airways and United Airlines — that now carries the telescope, its support systems, and the mission crew. The DLR designed, built and maintains the telescope which operates while flying at altitudes up to 45,000 feet at more than 650 mph.


Images above: Left: SOFIA soars over the snow-covered Sierra Nevada mountains with its telescope door open during a test flight. Right: Inside SOFIA during an observing flight at 40,000 feet. The mission crew, including telescope operators and scientists, sit facing the telescope at the back of the aircraft. The portion of the telescope that is inside the cabin is the blue round structure. The beige wall around the blue telescope structure is a pressure bulkhead that separates the open telescope cavity from the pressurized cabin, so the cabin environment feels similar to a commercial aircraft. Images Credits: Left: NASA/Jim Ross Right: NASA/DLR/Fabian Walker.

Aircraft modifications included cutting the hole for the telescope cavity, adding a new pressure bulkhead to separate the pressurized cabin from the cavity, and adding airflow ramps around the cavity that allow the plane to fly normally while the telescope door is open. Inside the cabin, mission control systems required for the observatory replaced the seats from the aircraft’s days as a passenger plane. The modifications and test flights took place in Waco, Texas and at NASA’s Armstrong Flight Research Center Hangar 703. About 20 people are aboard each flight to operate the aircraft, control the telescope and collect astronomical data.


Image above: SOFIA’s telescope, as seen during construction before its reflective aluminium coating was applied, reveals the honeycomb design that reduces its weight by 80%. Image Credits: NASA/Ron Strong.

The German-built telescope is made of a unique glass material that has almost zero thermal expansion, so the mirror is unaffected by the temperature changes between the warm ground-level air and the cold stratosphere. The back of the telescope has a honeycomb design to make it approximately 80 percent lighter than most telescopes of this size. An intricate stabilization system isolates the telescope from the aircraft’s movement, keeping it fixed on its observing target during overnight flights. SOFIA reached full operational capacity in 2014 and flies three or more times per week for 10 hours at a time. 

Astronomers are using SOFIA to study many different kinds of astronomical objects and phenomena, including:

- Star birth and death
- The formation of new solar systems
- Identification of complex molecules in space
- Planets, comets and asteroids in our solar system
- Nebulae and the ecosystems of galaxies
- Celestial magnetic fields
- Black holes at the center of galaxies



Image above: NASA’s airborne infrared observatories — the Learjet Observatory, the Kuiper Airborne Observatory and SOFIA — are pictured next to illustrations showing how the size of each telescope approximately compares to an adult. Image Credits: NASA/SOFIA/L. Proudfit.

NASA’s Ames Research Center in California’s Silicon Valley manages the SOFIA program, science and mission operations in cooperation with the Universities Space Research Association headquartered in Columbia, Maryland, and the German SOFIA Institute (DSI) at the University of Stuttgart. The aircraft is operated and maintained from NASA’s Armstrong Flight Research Center Hangar 703, in Palmdale, California.

Add-on for Flight Simulator X:

Image Credit: Orbiter.ch Aerospace

NASA & DLR Boeing 747/SP SOFIA Observatory repaint for FSX
https://simulators.jimdo.com/

Related links:

Stratospheric Observatory for Infrared Astronomy (SOFIA): https://www.nasa.gov/mission_pages/SOFIA/index.html

NASA's Kuiper Airborne Observatory: https://www.nasa.gov/vision/universe/watchtheskies/kuiper.html

NASA’s Armstrong Flight Research Center: https://www.nasa.gov/centers/armstrong/home/index.html

Images (mentioned), Text, Credits: NASA/SOFIA Science Center/Kassandra Bell.

Best regards, Orbiter.ch

Japanese Cargo Ship Arrives Thursday; U.S., Russian Crew Leaves Next Week













ISS - Expedition 56 Mission patch.

September 26, 2018

The Expedition 56 crew aboard the International Space Station awaits the arrival of new science experiments and crew supplies Thursday morning. One week later, three crew members will return to Earth after 197 days in space.

Japan’s H-II Transfer Vehicle-7 (HTV-7), also known as the “Kounotori,” is nearing the station and headed for a Thursday morning capture at 8 a.m. EDT. The HTV-7 is loaded with over five tons of science and supplies, including the new Life Sciences Glovebox and a half dozen lithium-ion batteries to upgrade the station’s power systems. NASA TV begins its live coverage of the capture activities Thursday at 6:30 a.m.


Image above: Commander Drew Feustel participates in an event inside Japan’s Kibo laboratory module aboard the International Space Station. Image Credit: NASA.

NASA astronauts Drew Feustel and Serena Auñón-Chancellor are finalizing several weeks of computer training today to capture the HTV-7. Feustel will be inside the cupola and command the Canadarm2 robotic arm to capture the Kounotori Thursday morning. Auñón-Chancellor will back up Feustel and monitor the Kounotori’s approach and rendezvous.

Meanwhile, Feustel and two other Expedition 56 crewmates are scheduled to depart the orbital laboratory on Oct. 4 just a week after the Kounotori arrives. Soyuz Commander Oleg Artemyev will lead the flight home inside the Soyuz MS-08 spacecraft flanked by Feustel and NASA astronaut Ricky Arnold.

International Space Station (ISS). Image Credit: NASA

The three departing crewmates have been packing up crew supplies, station hardware and science experiments to take back to Earth. The trio also practiced their Soyuz descent maneuvers and prepared themselves for the effects of returning to gravity. . Once the trio departs, Expedition 57 officially begins.

NASA astronaut Nick Hague and Soyuz Commander Alexey Ovchinin will launch and arrive one week later. During Expedition 57, the crew will conduct a set of spacewalks to install the new lithium-ion batteries delivered to the station on HTV-7.

Related links:

Expedition 56: https://www.nasa.gov/mission_pages/station/expeditions/expedition56/index.html

Expedition 57: https://www.nasa.gov/mission_pages/station/expeditions/expedition56/index.html

Life Sciences Glovebox: https://orbiterchspacenews.blogspot.com/2018/09/partnership-teamwork-enable-landmark.html

Spacewalks: https://www.nasa.gov/mission_pages/station/spacewalks

NASA TV: https://www.nasa.gov/nasatv

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

How a Tiny Curiosity Motor Identified a Massive Martian Dust Storm











NASA - Mars Science Laboratory (MSL) logo.

Sept. 26, 2018

There is no shortage of eyeballs, human and robotic, pointed at Mars. Scientists are constantly exploring the Red Planet from telescopes on Earth, plus the six spacecraft circling the planet from its orbit, and two roving its surface. So when dust filled the atmosphere during the recent planet-wide dust storm, observations were plentiful.


Animation above: Rotating globes from May 28 and July 1 show a global dust storm completely obscuring the surface of Mars. Animation Credits: NASA/JPL-Caltech/MSSS.

NASA’s Mars Reconnaissance Orbiter (MRO) provided the earliest insights on May 30 when it observed an accumulation of dust in the atmosphere near Perseverance Valley, where NASA’s Opportunity rover is exploring. The increasingly hazy storm, the biggest since 2007, forced Opportunity to shut down science operations by June 8, given that sunlight couldn’t penetrate the dust to power the rover’s solar panels. Scientists are anxiously waiting for the roving explorer to regain power and phone home.

Meanwhile, on June 5, evidence quietly materialized on the other side of the globe that the storm was growing and beginning to affect Gale Crater, the research site of NASA’s Curiosity rover. (The storm was officially classified as global on June 20.)

It came from an unexpected source: an actuator, or motor, that powers a lid to a funnel that takes in samples of powdered Martian rock dropped in by Curiosity’s drill. The samples then undergo chemical analysis by the portable Sample Analysis at Mars (SAM) chemistry lab, designed by scientists at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and built into Curiosity’s belly.

Benito Prats, a Goddard electromechanical engineer, noticed the dust storm slowly reaching Curiosity through the continuous temperature readings he collected from actuator sensors.


Image above: The left photo shows the deck of the Curiosity rover, on sol (Martian day) 36, or Sept. 10, 2012, which was about a month into its mission on Mars. The deck is clean, save for a few particles and a shadow of the MastCam, which snapped the photo. The photo on the right, taken on sol 2,068, or May 31, 2018, shows dirt particles, powder and dust on the rover deck, surrounding an actuator. Not all the dust comes from the recent storm, though. Mars is dusty in general, so most of the dust pictured has accumulated over six years. Sometimes particles are kicked in to the air when the rover drives, other times dust devils or a gust of wind lift the dust and deposit it on the rover deck. Image Credits: NASA/JPL-Caltech.

“All my charts showed the dust storm effect on the actuator because it’s exposed; it’s sitting out there on the rover deck,” said Prats. “All of a sudden, I saw the daytime temperature drop really quickly.”

At night, too, said Prats, he saw temperatures rising above normal levels. This happens during a dust storm because less sun penetrates the dusty atmosphere during the day, cooling the surface of the planet, while at night, the warmer, dusty atmosphere heats the ground. Other weather tools on the explorer, such as the Rover Environmental Monitoring Station, which measures air temperature, atmospheric pressure, and other environmental conditions, were also beginning to indicate accumulating dust.

Unlike solar-powered Opportunity, Curiosity is powered by a plutonium generator, so its operations were not affected by the dust shade. The temperature changes also didn’t affect SAM actuators — there are two sample funnels, in case one gets clogged — since they like warmer, less extreme temperatures.

SAM analyzes Martian rocks and soils in search of organic materials. In order for SAM to work properly, its actuators need to be at minus 40 degrees Celsius (minus 40 Fahrenheit). This is why Prats keeps a close eye on their temperature. When Martian temperatures in spring dip to minus 60 degrees Celsius (minus 76 Fahrenheit) at night, SAM heaters must warm up the motors to lift the funnel lid for sample drops.

SAM Actuator

Video above: This video was taken in January 2011 in the clean room at NASA’s Jet Propulsion Laboratory in Pasadena, California, by SAM lead mechanical engineer, Oren Sheinman, before NASA’s Curiosity rover was shipped to NASA’s Kennedy Space Center in Florida for launch. Both actuators are shown and both were tested to make sure they opened and closed without binding; in particular, mechanical engineers were making sure all parts were mounted correctly. The top of the funnel is covered with ultra-high-vacuum aluminum foil to prevent the few particles in the clean room from entering the sample path. The white surface is the rover deck that later is covered with Mars dust, and the markings on the cover are used to align the dropping mechanism, CHIMRA, at the center of the sample funnel. Video Credits: NASA/Benito Prats/Molly Wasser.

After Prats discovered the effects of the dust storm in his temperature data, he combined it with historic actuator temperature averages to estimate when the dust storm would abate.

“At sol 2,125 (July 28), I noticed a linear trend,” he said, “so I said OK, I can predict that sol 2,180 (Sept. 23) is going to be when we’re going to get out of the dust storm and the temperature will return back to normal, though I later updated that to sol 2,175 (Sept. 18).” His prediction was consistent with more formal ones, and matches recent actuator temperature readings, which were back to normal around Sept. 18, indicating that the dust over Gale Crater had settled by then. A majority of the dust also has settled at Perseverance Valley.


Images above: The chart on the first is showing temperatures for a SAM actuator, starting at Martian sol 2,055, which was May 18 on Earth. The diagonal lines that form a cone starting on sol 2,085 show Benito Prats’ predicted actuator temperature range through sol 2,180, or Sept. 23. The vertical blue lines that fill the cone are actual motor temperature readings. The dust storm was classified as global on June 20, or sol 2,088. By that point, the actuator temperature had changed drastically, as is clear in the relatively sudden narrowing of the chart, indicating cooler daytime temperatures and warmer night-time temperatures. The second chart is the same, but shows actual temperature readings through sol 2,180, or Sept. 23. Images Credits: NASA's Goddard Space Flight Center/Benito Prats/Molly Wasser.

Data from any source, even the most unexpected, are useful to planetary scientists, given we still don’t know why some Martian dust storms last for months and grow massive, while others stay small and last only a week.

Scientists hope to be able to forecast these global events, like they can forecast hurricanes on Earth, in order to better understand the planet’s current and past climate and to properly design robotic and human missions to the planet, NASA scientists say.

“There are some things about Mars that make it more predictable and some that make it less so than Earth,” said Scott D. Guzewich, a Goddard atmospheric scientist leading Curiosity's dust storm investigation.

Mars Science Laboratory (MSL) or Curiosity rover. Animation Credits: NASA/JPL-Caltech

“I can estimate, two years in advance, the temperature, air pressure, and whether there’s going to be dust or clouds in the air during the non-dusty season anywhere on the planet,” he said. “But during the dusty season, in locations that have dust storms, I can’t give you any prediction at all that there will be a dust storm on one day and not another.”

Related links:

Mars Reconnaissance Orbiter (MRO): https://mars.nasa.gov/mro/

Rover Environmental Monitoring Station: https://mars.nasa.gov/msl/mission/instruments/environsensors/rems/

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

Goddard Space Flight Center: https://www.nasa.gov/centers/goddard/home/index.html

Images (mentioned), Animations (mentioned), Video (mentioned), Text, Credits: NASA/Karl Hille/Goddard Space Flight Center, by Lonnie Shekhtman.

Greetings, Orbiter.ch

mardi 25 septembre 2018

Arianespace Flight VA243 Mission Success





















ARIANESPACE - Flight VA242 Mission poster / ARIANESPACE - 100th Ariane 5 logo.

September 25, 2018

100 + 300 = Arianespace and Ariane 5’s history-making success for three long-time customers


Image above: Ariane 5 ascends from the Spaceport’s ELA-3 launch zone on its 100th flight, carrying a dual payload of the Horizons 3e and Azerspace-2/Intelsat 38 telecommunications satellites. Image Credit: Arianespace.

Arianespace’s on-target mission with Horizons 3e and Azerspace-2/Intelsat 38 marked the milestone 100th flight of a heavy-lift Ariane 5, confirming this workhorse vehicle’s role as the launch services industry reference in reliability, flexibility and performance.

With the deployment of its latest two passengers during a 42-minute flight from the Spaceport in French Guiana, Ariane 5’s combined lift performance over these 100 missions exceeds 790 metric tons – including a total of 207 satellites for 68 customers around the globe. Overall, the launcher has achieved a remarkable 98.1% reliability rate during more than 22 years in service.

Arianespace Flight VA243 - Horizons 3e & Azerspace-2/Intelsat 38 Launch Sequence

Tonight’s success also marked the 300th flight by a member of the company’s family of launchers, in which Ariane 5 is joined by the medium Soyuz and lightweight Vega in side-by-side operations at the Spaceport.

“For Ariane 5 mission number #100, our heavyweight launcher has once more performed flawlessly. Congratulations to all!” said Arianespace CEO Stéphane Israël in his post-launch speech. “Ariane 5 joins Ariane 4 in the heavy-lift launcher hall of fame, with Ariane 4 having delivered 116 times. And we think Ariane 5 will deliver more.”

A success for loyal customers

Designated Flight VA243, today’s heavy-lift success continues long relationships of trust between Arianespace and the mission’s customers. Horizons 3e was released first in the flight sequence, being deployed from the upper slot in Ariane 5’s payload configuration, followed by Azerspace-2/Intelsat 38, located in the lower passenger position. Total lift performance to geostationary transfer orbit (GTO) was estimated at 10,827 kg.

Horizons 3e was lofted for a joint venture of Intelsat and SKY Perfect JSAT Corporation. Built by Boeing using Intelsat’s EpicNG design, it will provide coverage for aeronautical and maritime mobility, fixed and wireless operators, as well as mobility and government customers. It also is the first satellite in Intelsat’s EpicNG spacecraft series to feature entire Ku-band spot beams utilizing multiport amplifiers that optimize power across the spacecraft.

Horizons 3e

The spacecraft is a special payload on multiple fronts: Horizons 3e is the 60th Intelsat satellite to be launched by Arianespace, as well as the 20th for SKY Perfect JSAT. In addition, it is the 56th Boeing-built spacecraft orbited by the company to date.

“Arianespace is known for delivering, and we are very appreciative of another flawless mission,” stated Ken Lee, Intelsat’s Senior Vice President of Space Systems. “Ariane 5 has delivered 17 Intelsat satellites over the past 18 years, and we are thrilled that we could be part of Ariane 5’s 100th launch.”
Building on long-term cooperation

Azerspace-2/Intelsat 38 – built by SSL, a Maxar Technologies Company – offers 35 active transponders in Ku-band and has designed lifetime of more than 15 years. With today’s success, Arianespace has now orbited a total of 65 satellites produced by SSL.

Azerspace-2/Intelsat 38

Azerspace-2 will increase the coverage area and spectrum of services provided by Azercosmos, expanding on the current capacity of Azerspace-1 – the operator’s first relay platform, launched on an Arianespace Ariane 5 mission in February 2013. The spacecraft’s planned orbital position is only one degree away from the current Azerspace-1 orbital location at 46° East, which creates favorable opportunities for existing and new customers to start expanding their current satellite solutions.

The satellite will offer enhanced capacity, coverage and service offerings to support growing demand in the region for Direct-to-Home (DTH), government and network services in Europe, Central and South Asia, the Middle East and Sub-Saharan Africa.

Azercosmos Vice Chairman Dunay Badirkhanov thanked Arianespace for a “spectacular launch and an exciting journey,” adding that Arianespace’s launch services have enabled Azercosmos to become a leading satellite services operator in its region of the world.

Arianespace TV - VA243 Sucessful Mission

In his speech from the Spaceport’s Jupiter control room, he explained that Azercosmos also is contributing to the development of human resources in the country by training a new generation of skilled personnel – including satellite engineers. “Today, there are students among us from the leading universities of Azerbaijan. In some years, they may be standing here delivering a congratulatory speech after another successful launch.”

Intelsat 38 will provide Ku-band capabilities and deliver continuity of service for the Intelsat 12 satellite located at 45° East. The satellite will host leading Direct-to-Home television platforms for the fast-growing Central and Eastern Europe and Asia-Pacific regions, as well as provide critical broadband connectivity for corporate network and government services in Africa. It is the 61st Intelsat spacecraft lofted by Arianespace.

Related link:

ARIANESPACE: http://www.arianespace.com/

Images, Videos, Text, Credits: ARIANESPACE/ EpicNG/Azerspace/SSL.

Best regards, Orbiter.ch

Opportunity Emerges in a Dusty Picture














NASA - Mars Reconnaissance Orbiter (MRO) logo/ NASA - Mars Exploration Rover B (MER-B) patch.

Sept. 25, 2018

NASA still hasn't heard from the Opportunity rover, but at least we can see it again.


Image above: NASA's Opportunity rover appears as a blip in the center of this square. This image taken by HiRISE, a high-resolution camera onboard NASA's Mars Reconnaissance Orbiter, shows the dust storm over Perseverance Valley has substantially cleared. Image Credits: NASA/JPL-Caltech/Univ. of Arizona.

A new image produced by HiRISE, a high-resolution camera aboard NASA's Mars Reconnaissance Orbiter (MRO), shows a small object on the slopes of the Red Planet's Perseverance Valley. That object is Opportunity, which was descending into the Martian valley when a dust storm swept over the region a little more than 100 days ago.

The storm was one of several that stirred up enough dust to enshroud most of the Red Planet and block sunlight from reaching the surface. The lack of sunlight caused the solar-powered Opportunity to go into hibernation.

Mars Exploration Rover (MER). Image Credits: NASA/JPL-Caltech

The rover's team at NASA's Jet Propulsion Laboratory in Pasadena, California, hasn't heard from it since. On Sept. 11, JPL began increasing the frequency of commands it beams to the 14-year-old rover.

The tau -- a measurement of how much sunlight reaches the surface -- over Opportunity was estimated to be a little higher than 10 during some points during the dust storm. The tau has steadily fallen in the last several months. On Thursday, Sept. 20, when this image was taken, tau was estimated to be about 1.3 by MRO's Mars Color Imager camera.

This image was produced from about 166 miles (267 kilometers) above the Martian surface. The white box marks a 154-foot-wide (47-meter-wide) area centered on the rover.

Mars Reconnaissance Orbiter (MRO). Image Credits: NASA/JPL-Caltech

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

For more, visit: https://www.uahirise.org/ESP_056955_1775

Updates about Opportunity can be found here: https://mars.nasa.gov/mer/mission/status.html

Mars Exploration Rovers (Spirit and Opportunity): https://www.nasa.gov/mission_pages/mer/index.html

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

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

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