mercredi 14 janvier 2015

Latest images received from comet 67P/Churyumov-Gerasimenko by Rosetta












ESA - Rosetta Mission patch.

January 14, 2015

This four-image mosaic comprises images taken from a distance of 27.5 km from the centre of Comet 67P/Churyumov-Gerasimenko on 8 January. The image resolution at this distance is about 2.3 m/pixel and the individual 1024 x 1024 frames measure about 2.4 km across. The mosaic measures 4.3 x 3.9 km.

Comet on 8 January 2015 – NavCam

Image above: This four-image mosaic comprising images taken on 8 January 2015. Rotation and translation of the comet during the imaging sequence make it difficult to create an accurate mosaic, so always refer to the individual images before drawing conclusions about any strange structures or low intensity extended emission. Image Credits: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0.

In this view the smaller of the comet’s two lobes is to the right, presenting a side-on look into the large, roughly 1 km-wide depression towards the edge of the mosaic. The rugged outline of the smaller lobe can be traced into the shadows, creating a nice contrast against the smooth neck region in the centre of the image. As noted in this portion of the neck has some particularly interesting features, such as the bright, exposed cliffs, the curved trough-like features and dark markings in the dusty layer.


Image above: This four-image mosaic comprising images taken on 8 January 2015. Rotation and translation of the comet during the imaging sequence make it difficult to create an accurate mosaic, so always refer to the individual images before drawing conclusions about any strange structures or low intensity extended emission. Image Credits: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0.

To the left, the image offers a striking view of the large comet lobe, in particular the steep, layered cliff face that towers above a smoother, dust-covered ledge. At its edge, it appears as though some of the dust may have slipped away. Towards the background, ridges seem to cut through the terrain, while several flat-topped plateaus are set along the horizon.

For more information about Rosetta mission, visit: http://www.esa.int/Our_Activities/Space_Science/Rosetta

Images (mentioned), Text, Credit: ESA.

Greetings, Orbiter.ch

A year on-station for Gaia












ESA - Gaia Mission patch.

January 14, 2015

Time flies when you’re mapping a billion stars!

One year ago, Gaia performed its last major orbit insertion burn and was stable at 'L2'.


Image above: Gaia is an ambitious mission to chart a three-dimensional map of our Galaxy, the Milky Way, in the process revealing the composition, formation and evolution of the Galaxy. Credit: ESA–D. Ducros, 2013.

After a smooth, but operationally intense lift-off, LEOP (launch and early orbit phase) and transfer phase, in which Gaia travelled the 1.5 million km from Earth to the point at which the sky survey will be done, the work to start Gaia’s mapping task was only just beginning.

The five thrusters used to perform the orbit insertion are commanded to stop firing and there are smiles in the control room at ESOC as the telemetry on the screens confirm the last planned ‘critical operation’ is successfully completed.

Thruster Firings

Earlier, Gaia’s operators had to perform a number of critical operations in the initial post-launch period: the first autonomous flight activation; sun-shield deployment and three orbit manoeuvres – when the thrusters were heavily used – all between 2 and 27 days after launch.

Had these gone wrong, the mission operations team would have been in a race against the clock to stop Gaia drifting off into interplanetary space.

Today we are one year on from the last of these.

The blue line in the Earth-centered plot below shows the correct trajectory (i.e. the nominal case when the manoeuvre worked) and the green shows what would have happened without this manoeuvre (drift around the Earth-Moon system followed by escape into interplanetary space).


Graphic above: Gaia L2 arrival - worst case scenario. Graphic Credit: ESA.

Now that this activity was over, the operations team could fully focus on the commissioning phase, testing and configuring the spacecraft and payload operations until system performance was ready to perform science.

This was not time-critical, but was technically demanding, and this phase would eventually last six months.

Gaia is a one-off, purpose-built spacecraft that is capable of mapping the positions of one billion stars to unprecedented precision (to the micro-arc-second level, comparable to the width of a smart phone on the Moon as viewed from Earth). This performance is far beyond anything previously achieved, and the Gaia spacecraft is a marvel of engineering in its own right.

Spacecraft are complex

Spacecraft such as Gaia are complex machines, which have layered operational modes.

The spacecraft can be flown and operated, performing the more basic tasks, with a subset of service module units on and working. Just like the tip of a pyramid can only be placed on top after all other stones have been laid, all on-board prime units must be switched on and correctly configured for full performance. This, together with checking a number of redundant units and functions, is the task of teams on ground during the commissioning phase.

The Gaia spacecraft has a relatively large fraction of ‘bespoke’ units i.e. custom designed, due largely to the incredible precision requirements. Not the least of these are the telescopes and camera.

Gaia’s camera is the most impressive ever flown in space, containing 106 CCDs, which are around 90% light efficient (a CCD in a typical digital camera is around 20% efficient).

Inside Gaia's billion-pixel camera

These have to be linked to the on-board attitude control system to achieve the needed and incredible precision for mapping the stars.

Gaia must rotate once every 6 hours to scan the heavens and this rate is so precisely controlled that the error is equivalent to one rotation every 410 years. There are (and can be) no moving parts on board, so the data is downlinked through a novel electromagnetically steerable antenna.

Attitude control is provided by a micro propulsion system that has its first flight use with Gaia. This delivers micro-Newton levels of thrust primarily to oppose the quantum mechanical force exerted by sunlight falling onto the sunshield. An atomic clock is used for precise time-stamping, which in fact allows controllers to see the time dilation effects from Einstein’s Theory of General Relativity.

Just after entry into the operational orbit, most of these hardware units were either off or had hardly been used at all.

Solving problems with teamwork

One year ago, the critical phases were over and the operations team began focusing on the complex task of bringing the spacecraft up to full performance.

In terms of what was planned, this consisted of an iterative phase where teams on the ground send commands to move the mirrors and adjust the spacecraft spin rate and then industry (i.e. the spacecraft manufacturer) and the mission science teams analysed the results before the next tuning cycle. The other major element planned was the tuning of Gaia’s seven powerful video processing units, each connected to a row of the camera’s CCDs, responsible for identifying and characterizing the stars that will make up Gaia’s map.

These tasks progressed well, but almost immediately after orbit insertion some problems became apparent.

First noticed through an apparent dimming of the on-board laser used to track the angle between the telescope mirrors, and later confirmed by data from the stars themselves, ice was unexpectedly building up and had to be dealt with .

Also apparent was more background light than expected .

These issues, like many others, were dealt with and solved in a series of brainstorming review meetings between experts, some of which required in-orbit special operations to be developed and executed to provide the necessary data. For example, Gaia’s normally rock-stable sun-attitude was changed twice in special operations designed to characterise the stray-light problem.

Examples elsewhere from the spacecraft commissioning period included a micro-propulsion thruster with unexpected performance levels and a back-up chemical thruster that had a failed valve (meaning it was permanently lost).

Teamwork has been critical

Again, teamwork in brainstorming review meetings was critical to solving these issues. The on-board software could be quickly reprogrammed to match the new performance of the micro-propulsion thruster and the on-board protection software was changed to make sure the system would never try to use the chemical thruster that had failed (for this was a thruster present in case the spacecraft was in trouble and needed to put itself into ‘Safe Mode’).


Image above: An artist’s impression of a Type Ia supernova – the explosion of a white dwarf locked in a binary system with a companion star. Image Credit: ESA/ATG medialab/C. Carreau.

By the end of the commissioning phase, the teamwork between the ESA operations, project and science teams together with the industry experts at AirbusDS and the wider Gaia scientific community organised into the Data Processing and Analysis Consortium (DPAC) had delivered the spacecraft in excellent shape.

The spacecraft was correctly configured and the software of the majority of on-board units had been changed based on the lessons learned to date. In getting to this stage, approximately 400 000 telecommands had been sent by ground teams.

Shortly after the commissioning ended, a new Survival Mode was activated on board, using thrusters that are normally used only for orbit manoeuvres. This meant that single failure tolerance had been fully restored, even with a permanently lost thruster.

The mapping begins

By July 2014, Gaia was busy mapping parts of the sky that had been calibrated by ground telescopes, before its nominal scanning mode was entered in September.

At this point Gaia was working so well that it was producing more data than originally foreseen, since it was able to see stars fainter than required. Towards the end of the year, operators had to come up with a method to partially automate ground operations allowing Gaia to take advantage of more ground station time and expand its mapping data set.

It’s been a busy first year for Gaia, but at the one-year point there’s a good sense of achievement.

The science data are now coming down in huge quantities (11 billion camera transits were recorded by the one-year launch anniversary), with anticipation slowly building for what Gaia may find in the coming years.

But even before the first map release next year, Gaia is already making discoveries (see "Gaia discovers its first supernova" http://orbiterchspacenews.blogspot.ch/search?q=Gaia+discovers+its+first+supernova).

Happy anniversary Rosetta!

Rosetta update provided by Gaia Spacecraft Operations Manager Dave Milligan at ESOC.

Related link:

AirbusDS: http://www.space-airbusds.com/en/programme/gaia.html

For more information about Gaia mission, visit: http://www.esa.int/Our_Activities/Space_Science/Gaia

Images (mentioned), Graphic, Video, Text, Credit: European Space Agency (ESA).

Best regards, Orbiter.ch

Tracking a ghost mission 238 million km away












ESA - Venus Express Mission patch.

January 14, 2015

On 16 December, ESA's hugely successful Venus Express mission came to an end after it exhausting its remaining propellant as of 28 November (see "Venus Express goes gently into the night" http://orbiterchspacenews.blogspot.ch/search?q=Venus+Express+goes+gently+into+the+night).

No more fuel means no more ability to control the spacecraft and keep the high-gain antenna (HGA) pointed toward Earth, which in turn means there is no way to upload telecommands nor receive telemetry (including the on-board housekeeping data).

Basically, Venus Express is ghosting along in its orbit, with the pericentre height (height of closest altitude above the surface) during each orbit steadily decaying due to gravity and natural perturbations.

Visualisation of Venus Express during the aerobraking in 2014. Image Credits: ESA/C. Carreau

But while no more science data can be gathered, and no more attempts to send commands will be made, the operations team at ESOC are able to continue monitoring radio signals from the spacecraft; they can 'see' the X-band carrier wave being transmitted from the spacecraft's high-gain antenna despite the fact that it is not pointed at Earth, although this, too, is steadily dropping off.

The intrepid craft may be stuck in Sun-acquisition mode. This could mean it is maintaining a coarse pointing with the solar arrays and HGA pointed approximately toward the Sun, within perhaps 5 degrees or so.

But whether pointing toward the Sun or not, the HGA is not pointing toward our ground station on Earth, and as Venus and Earth move in their orbits, this off-Earth pointing (see 'Sun-spacecraft-Earth angle' in the chart) is becoming larger. This means that the strength of the received carrier signal is steadily declining.

"On New Year's day, we saw a weak but detectable signal level and could lock onto it for most of the almost-5-hour tracking pass using the Cebreros deep-space tracking station," says Rick Blake, Venus Express spacecraft operations engineer at ESOC.

"But on 7 January, we only got carrier lock on a more weakened signal for just five percent of the pass; on 8 January, we were back to a good lock for most of the pass, so it's definitely an unpredictable situation."

"We plan to continue monitoring the signal level in January until we see it has disappeared for good," says Blake.

VEX carrier lock 1-8 Jan 2015

In an earlier email, Håkan Svedhem, ESA's Venus Express project scientist, said he expected the pericentre altitude to drop to about 130km around 12 January and 120km around 20 January.

"My personal guess is that the spacecraft will start breaking up soon after that."

This will be unseen by any human, and it appears that we'll never know when it actually happens.

"It will be destroyed in the atmosphere most likely toward the end of January or early February," says Patrick Martin, ESA’s Venus Express mission manager.

But while the spacecraft will burn up in the dense Venusian atmosphere – experiencing a lonely and poignant end – the science and operations teams on Earth will begin work on the important post-operations phase.

This will ensure that the vital science and flight data recorded during eight years of exploring Venus are available to current and future researchers, making a fitting legacy for such a successful mission.

For more information about Venus Express mission, visit: http://www.esa.int/Our_Activities/Space_Science/Venus_Express

Image (mentioned), Graphic, Text, Credit: ESA.

Cheers, Orbiter.ch

Asteroid to Fly By Earth Safely on January 26










Asteroid watch logo.

January 14, 2015

An asteroid, designated 2004 BL86, will safely pass about three times the distance of Earth to the moon on January 26. From its reflected brightness, astronomers estimate that the asteroid is about a third of a mile (0.5 kilometers) in size.

Graphic depicts the trajectory of asteroid 2004 BL86

The flyby of 2004 BL86 will be the closest by any known space rock this large until asteroid 1999 AN10 flies past Earth in 2027. At the time of its closest approach on January 26, the asteroid will be approximately 745,000 miles (1.2 million kilometers) from Earth.

Asteroid Watch: For more information about asteroids and near-Earth objects, visit: http://www.jpl.nasa.gov/asteroidwatch and http://www.nasa.gov/asteroid . Updates about near-Earth objects are also available by following AsteroidWatch on Twitter at http://www.twitter.com/asteroidwatch .

Near-Earth Object Program Office: http://neo.jpl.nasa.gov/

Graphic, Text, Credit: NASA.

Greetings, Orbiter.ch

Crew Safe After Alarm on Station












ISS - International Space Station patch.

January 14, 2015

(STS-134) view of the International Space Station (ISS). Image Credit: NASA TV

The Expedition 42 crew members are safe and in good shape inside the Russian segment of the International Space Station following an alarm in the U.S. segment at about 4 a.m. EST.

Flight controllers in Mission Control at NASA’s Johnson Space Center in Houston saw an increase in pressure in the station’s water loop for thermal control system B then later saw a cabin pressure increase that could be indicative of an ammonia leak in the worst case scenario. Acting conservatively to protect for the worst case scenario, the crew was directed to isolate themselves in the Russian segment while the teams are evaluating the situation. Non-essential equipment in the U.S. segment of the station was also powered down per the procedures.

In an exchange at 7:02 a.m. with Expedition 42 Commander Barry Wilmore of NASA, spacecraft communicator James Kelly said flight controllers were analyzing their data but said it is not yet known if the alarm was actually triggered by a leak or whether the situation was caused by a faulty sensor or by a problem in a computer relay box that sends data and commands to various systems on the station.

NASA TV will provide a live update at 7:45 a.m. ET at http://www.nasa.gov/nasatv

For more information about the International Space Station (ISS), visit: http://www.nasa.gov/mission_pages/station/main/index.html

Image (mentioned), Text, Credit: NASA.

Greetings, Orbiter.ch

mardi 13 janvier 2015

Space Station Crew Opens Dragon for Business










ISS - Expedition 42 Mission patch.

13 January 2015

The hatches to Dragon were opened for business Tuesday morning at 3:23 a.m. EST and the crew began unpacking critical gear that will support 256 science experiments. The SpaceX commercial cargo craft was attached Monday to the Harmony module at 8:54 a.m.

Read more about the arrival of the SpaceX CRS-5 mission: http://orbiterchspacenews.blogspot.ch/2015/01/dragon-attached-to-space-station.html


Image above: Italian astronaut Samantha Cristoforetti takes a peek inside the just opened Dragon commercial cargo craft. Credit: NASA TV.

One experiment that was immediately set up by Flight Engineer Terry Virts was the Micro-5 study. That experiment observes microorganisms as a model for humans so scientists can understand changes in a crew member’s immune system and the risk of infectious disease in space.

Read more about Micro-5: http://www.nasa.gov/mission_pages/station/research/experiments/810.html

For more information about the International Space Station (ISS), visit: http://www.nasa.gov/mission_pages/station/main/index.html

Image (mentioned), Text, Credit: NASA.

Best regards, Orbiter.ch

First Notable Solar Flare of 2015












NASA - Solar Dynamics Observatory patch.

13 January 2015


The sun emitted a mid-level solar flare, peaking at 11:24 p.m. EST on Jan. 12, 2015. NASA’s Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event.

Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel.

For more information about Solar Dynamics Observatory (SDO), visit: http://www.nasa.gov/mission_pages/sdo/main/

Image, Text, Credits: NASA/SDO.

Greetings, Orbiter.ch