OrbitalHub

ESA dixit:

“This animation shows changes in Earth’s magnetic field from January to June 2014 as measured by ESA’s Swarm trio of satellites.

The magnetic field protects us from cosmic radiation and charged particles that bombard Earth, but it is in a permanent state of flux. Magnetic north wanders, and every few hundred thousand years the polarity flips so that a compass would point south instead of north.

Moreover, the strength of the magnetic field constantly changes — and it is currently showing signs of significant weakening.

The field is particularly weak over the South Atlantic Ocean — known as the South Atlantic Anomaly. This weak field has indirectly caused many temporary satellite ‘hiccups’ (called Single Event Upsets) as the satellites are exposed to strong radiation over this area.

More about Swarm: http://www.esa.int/swarm“

Credit: ESA/Dot2Dot

NASA Goddard dixit:

“This supercomputer simulation shows one of the most violent events in the universe: a pair of neutron stars colliding, merging and forming a black hole. A neutron star is the compressed core left behind when a star born with between eight and 30 times the sun’s mass explodes as a supernova. Neutron stars pack about 1.5 times the mass of the sun — equivalent to about half a million Earths — into a ball just 12 miles (20 km) across.

As the simulation begins, we view an unequally matched pair of neutron stars weighing 1.4 and 1.7 solar masses. They are separated by only about 11 miles, slightly less distance than their own diameters. Redder colors show regions of progressively lower density.

As the stars spiral toward each other, intense tides begin to deform them, possibly cracking their crusts. Neutron stars possess incredible density, but their surfaces are comparatively thin, with densities about a million times greater than gold. Their interiors crush matter to a much greater degree densities rise by 100 million times in their centers. To begin to imagine such mind-boggling densities, consider that a cubic centimeter of neutron star matter outweighs Mount Everest.

By 7 milliseconds, tidal forces overwhelm and shatter the lesser star. Its superdense contents erupt into the system and curl a spiral arm of incredibly hot material. At 13 milliseconds, the more massive star has accumulated too much mass to support it against gravity and collapses, and a new black hole is born. The black hole’s event horizon — its point of no return — is shown by the gray sphere. While most of the matter from both neutron stars will fall into the black hole, some of the less dense, faster moving matter manages to orbit around it, quickly forming a large and rapidly rotating torus. This torus extends for about 124 miles (200 km) and contains the equivalent of 1/5th the mass of our sun. The entire simulation covers only 20 milliseconds.

Scientists think neutron star mergers like this produce short gamma-ray bursts (GRBs). Short GRBs last less than two seconds yet unleash as much energy as all the stars in our galaxy produce over one year.

The rapidly fading afterglow of these explosions presents a challenge to astronomers. A key element in understanding GRBs is getting instruments on large ground-based telescopes to capture afterglows as soon as possible after the burst. The rapid notification and accurate positions provided by NASA’s Swift mission creates a vibrant synergy with ground-based observatories that has led to dramatically improved understanding of GRBs, especially for short bursts.

The scientific paper this simulation is a part of can be found here: http://arxiv.org/abs/1001.3074“

Credit: David Link/Luciano Rezzolla/Michael Koppitz

 

NASA dixit:

“NASA’s Orion spacecraft is built to take humans farther than they’ve ever gone before. Orion will serve as the exploration vehicle that will carry the crew to space, provide emergency abort capability, sustain the crew during the space travel, and provide safe re-entry from deep space return velocities.

On December 4, 2014, Orion will launch atop a Delta IV Heavy rocket from Cape Canaveral Air Force Station’s Space Launch Complex Flight Test on the Orion Flight Test: a two-orbit, four-hour flight that will test many of the systems most critical to safety.

The Orion Flight Test will evaluate launch and high speed re-entry systems such as avionics, attitude control, parachutes and the heat shield. In the future, Orion will launch on NASA’s new heavy-lift rocket, the Space Launch System. More powerful than any rocket ever built, SLS will be capable of sending humans to deep space destinations such as an asteroid and eventually Mars. Exploration Mission-1 will be the first mission to integrate Orion and the Space Launch System.”

Credit: NASA

ESA dixit:

“This short movie tells the story of Rosetta’s journey through the Solar System and its exploration of Comet 67P/Churyumov–Gerasimenko so far, through the voices of some of the many people involved in this exciting mission.

ESA’s Rosetta spacecraft was launched in March 2004 and has chased down the comet for 10 years, reaching it on 6 August 2014. It is the first space mission to orbit a comet and to attempt a soft landing. It will also be the first mission to journey with a comet as they swing around the Sun throughout 2015.

In the last 10 years Rosetta has made three flybys of Earth and one of Mars, and passed by and imaged asteroids Steins and Lutetia. In June 2011, Rosetta was placed into deep-space hibernation as it cruised nearly 800 million kilometres from the warmth of the Sun, close to the orbit of Jupiter. This was necessary because not enough energy could be generated by the solar panels to keep all the spacecraft systems operating. On 20 January 2014, Rosetta woke up from hibernation and continued its journey towards the comet.

Rosetta first viewed its target from a distance in 2011. After the wake-up, the first sight of the comet came in March 2014. Since then, Rosetta scientists have been following the comet’s activity, studying it with various instruments on board. As Rosetta drew closer and closer in July, the complex shape of this double-lobed object was revealed.

After Rosetta arrived at the comet in August, it started mapping the surface in greater detail, leading to the selection of a target for the lander, Philae, in September 2014. The site, now named Agilkia after an island on the Nile river, is located on the smaller lobe of the comet.

Rosetta is scheduled to release Philae on 12 November and, seven hours later, the lander is expected to reach the comet’s surface.

Acknowledgements: The images of the comet were taken with the OSIRIS camera (ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA) and with the navigation camera (ESA/Rosetta/NavCam) on Rosetta; the self-portraits were taken with the CIVA instrument on Philae (ESA/Rosetta/Philae/CIVA); the ground-based images of the comet were taken using the European Southern Observatory’s Very Large Telescope in Chile. The images of asteroids Steins and Lutetia were also taken with the OSIRIS camera.”

Credit: ESA

ESA dixit:

“Could astronauts one day be printing rather than building a base on the Moon? In 2013 ESA, working with industrial partners, proved that 3D printing using lunar material was feasible in principle. Since then, work continues to investigate the technique. The shielding against radiation provided by a 3D-printed block of simulated lunar regolith was measured, providing important inputs for next-stage designs… Soon the Agency is due to investigate another lunar 3D printing method, harnessing concentrated sunlight to melt regolith rather than using a binding liquid.

But how might lunar 3D printing one day be used in practice? Foster+Partners, contributing architectural concepts for the original study, put together this outline of a hypothetical mission to 3D-print an entire a lunar base, illustrating the design factors that steered them in their work. The rim of Shackleton Crater at the lunar south pole was chosen for the base location. The Moon’s rotation is such that the Sun only grazes its poles at low angles. The result is a near-constant ‘peak of eternal light’ along the rim of Shackleton Crater, beside regions of permanent shadow. Building in the vicinity of such a site would offer plentiful solar power, and relief from the extremes of heat and cold found across the rest of the Moon.

In reality any lunar base remains firmly on the drawing board, but each small step forward in research makes future lunar colonisation a little more feasible. In November 2014 more than 350 experts came together for a two-day Additive Manufacturing for Space Applications workshop at ESA’s ESTEC technical centre in Noordwijk, the Netherlands. They discussed the potential of 3D printing – also known as Additive Manufacturing – to transform the way the space industry operates and begin preparing common standards for its use.”

Read more about 3D-printing using Lunar soil…

Credit: ESA/Foster+Partners

Orbital’s statement regarding the ORB-3 launch mishap:

(Dulles, VA 28 October 2014) – Orbital Sciences Corporation (NYSE: ORB), one of the world’s leading space technology companies, confirms that today’s Antares rocket launch from NASA’s Wallops Flight Facility was not successful. Shortly after lift-off from the Mid-Atlantic Regional Spaceport Pad 0A at 6:22 p.m. (EDT), the vehicle suffered a catastrophic failure. According to NASA’s emergency operations officials, there were no casualties and property damage was limited to the south end of Wallops Island. Orbital has formed an anomaly investigation board, which will work in close coordination with all appropriate government agencies, to determine the cause of today’s mishap.

“It is far too early to know the details of what happened,” said Mr. Frank Culbertson, Orbital’s Executive Vice President and General Manager of its Advanced Programs Group. “As we begin to gather information, our primary concern lies with the ongoing safety and security of those involved in our response and recovery operations. We will conduct a thorough investigation immediately to determine the cause of this failure and what steps can be taken to avoid a repeat of this incident. As soon as we understand the cause we will begin the necessary work to return to flight to support our customers and the nation’s space program.”

Orbital will provide more information as it becomes available and is verified.

Orbital’s update on October 29:

Early this morning, range officials performed an aerial survey of the launch facilities and surrounding areas at NASA’s Wallops Flight Facility where yesterday’s failure of the Antares rocket occurred after it lifted off from the Mid-Atlantic Regional Spaceport’s Pad 0A. Shortly after, a team of representatives from NASA, MARS and Orbital entered the launch site to perform a preliminary assessment of the launch complex and related facilities. The overall findings indicate the major elements of the launch complex infrastructure, such as the pad and fuel tanks, avoided serious damage, although some repairs will be necessary. However, until the facility is inspected in greater detail in the coming days, the full extent of necessary repairs or how long they will take to accomplish will not be known.

NASA has posted aerial views of the launch pad taken earlier today here.

Also today, Orbital made progress forming a permanent Accident Investigation Board (AIB) comprised of company officials, along with representatives from NASA and the NTSB, with the FAA providing overall oversight of the process. Initially, Mr. Rich Straka, Senior Vice President and Deputy General Manager of Orbital’s Launch Systems Group, served as the interim chairman to begin the investigation process immediately after the launch mishap. Today, Orbital appointed Mr. Dave Steffy, Senior Vice President and Chief Engineer of the company’s Advanced Programs Group, a highly experienced engineer well-versed in launch vehicle engineering and operations, to serve as the permanent chairman of the AIB.

No follow-on press conferences are planned at this time. Further updates on the situation and the progress of the ongoing investigation will be provided as they are available.

Orbital’s update on October 30:

Launch Site Status:

Based on initial sweeps conducted by an Orbital safety team, it appears a significant amount of debris remains on the site and it is likely substantial hardware evidence will be available to aid in determining root cause of the Antares launch failure. Some of the Cygnus cargo has also been found and will be retrieved as soon as we have clearance to do so to see if any survived intact. After up close visual inspections by the safety team, it still appears the launch site itself avoided major damage. There is some evidence of damage to piping that runs between the fuel and commodity storage vessels and the launch mount, but no evidence of significant damage to either the storage vessels or launch mount. Detailed evaluations by MARS and their engineering team will occur in the next couple of days. An Orbital-led team has begun cataloging and documenting the location of all pieces of debris over the next several days after which the debris will be relocated to storage bays on the island for further evaluation.

Antares Data Review:

Telemetry data has been released to Orbital and our engineers presented a very quick look assessment to the Accident Investigation Board at the end of the day. It appears the Antares vehicle had a nominal pre-launch and launch sequence with no issues noted. All systems appeared to be performing nominally until approximately T+15 seconds at which point the failure occurred. Evidence suggests the failure initiated in the first stage after which the vehicle lost its propulsive capability and fell back to the ground impacting near, but not on, the launch pad. Prior to impacting the ground, the rocket’s Flight Termination System was engaged by the designated official in the Wallops Range Control Center.

Orbital’s update on November 3:

Over the weekend, Orbital confirmed the participation of the following individuals who will serve on the Antares launch failure Accident Investigation Board (AIB), which is being led by Orbital under the oversight of the Federal Aviation Administration (FAA). The composition of the AIB is as follows:

Chairman: David Steffy, Chief Engineer of Orbital’s Advanced Programs Group.

Members: David Swanson, Senior Director of Safety and Mission Assurance for Orbital’s Technical Operations organization; Wayne Hale, Independent Consultant and Former NASA Space Shuttle Program Manager; David Cooper, Member of Orbital’s Independent Readiness Review Team for the company’s Launch Systems Group; Eric Wood, Director of Propulsion Engineering for Orbital’s Launch Systems Group; Tom Costello, Launch Vehicle Assessment Manager in the International Space Station Program at NASA’s Johnson Space Center; Matt Lacey, Senior Vehicle Systems Engineer for NASA’s Launch Services Program.

FAA Oversight Team: Michael S. Kelly, Chief Engineer, FAA Office of Commercial Space Transportation; Marcus Ward, Mishap Response Coordinator, FAA Office of Commercial Space Transportation.

Antares Data Review:

The AIB is initially focused on developing a “fault tree” and a timeline of the important events during the launch sequence. Due to the large amount of data available, the AIB is able to work with a rich source of information about the launch. One of the initial tasks for the AIB is to reconcile the data from multiple sources, a process that is now underway, to help create the launch sequence timeline.

Launch Site Status:

Over the weekend, Orbital’s Wallops-based Antares personnel continued to identify, catalogue, secure and geolocate debris found at the launch site in order to preserve physical evidence and provide a record of the launch site following the mishap that will be useful for the AIB’s analysis and determination of what caused the Antares launch failure. The debris is being taken to a NASA facility on Wallops Island for secure and weather resistant storage.