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Rosetta mission preview – Part 3: deep-space hibernation

4/28/2014

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PictureRosetta - ESA's historic comet-chasing mission.
In the first two parts of this mission preview (see blog posts for March 18 and March 31, 2014), we looked briefly at the overall mission objectives of the Rosetta programme, some physical characteristics of the spacecraft, and the major events during its journey from launch in 2004 to its fly-by of asteroid Lutetia in July 2010.  
 
Beyond this encounter, Rosetta’s orbit took the spacecraft to a maximum distance from the Sun of about 800 million km (5.3 AU), beyond the orbit of Jupiter.  As mentioned in Part 1, the primary electrical power onboard is produced by solar arrays, which
convert solar energy into electricity. 
However, as Rosetta moved further away from the Sun, the amount of power the arrays produced dropped off. 
The rate at which this happens is driven by something called an ‘inverse square law’, but there is also a factor governed by temperature – the arrays’ efficiency increases as temperature decreases.  For an explanation of the factors which govern the conversion of solar energy into electrical power see pages 179-183 of the book How Spacecraft Fly.  Cutting a long story short, and doing a simple calculation (taking account of the inverse square law, but not of the temperature effects), shows that if the Rosetta arrays can produce 840 W of electrical power at a distance from the Sun of 3.2 AU (see Part 1), then at maximum distance the power level drops to about 300 W.  Given that the spacecraft needs at least a total of about 400 W to maintain full operation, there is a requirement to introduce a new operational mode (referred to as ‘hibernation’) in which power consumption is severely reduced.  Consequently, in June 2011 the mission operators began a process of putting Rosetta into a state of deep-space hibernation for 2 ½ years until 2014, when the spacecraft would again be close enough to the Sun to sustain full operation.

PictureNASA's Deep Space Antenna at Canberra, Australia.
One of the first requirements was to put the spacecraft (which is nominally 3-axis stabilised –see Chapter 8 of the book) into a gentle spin using the attitude control subsystem.  A spin rate of around 1 rpm was set up about an axis directed toward the inner Solar System, and the Sun in particular.  The axis about which the spacecraft spins becomes inherently stable in terms of pointing direction, so in this case the operators could be assured that the large solar arrays would remain
presented to the Sun during the period of hibernation.  Consequently, solar power, albeit at a reduced level, could be guaranteed during hibernation.  Following on from this, all electrical payloads and subsystems were progressively shut down, with the exception of the onboard computer (OBC) and the crucial heater components of the thermal control subsystem.  

The onboard computer’s operation was required so a wake-up alarm could be set, and so that the process of bringing the spacecraft back to normal operation could be achieved at the end of the hibernation period.  The heater systems were also controlled autonomously by the OBC to ensure critical spacecraft elements were maintained within acceptable temperature limits – for example, the OBC itself and the liquid propellant tanks and fuel lines (to prevent them from freezing).  During the 2 ½ years of hibernation, the power level steadily dropped as distance from the Sun increased.  Then after aphelion (maximum distance from the Sun), this power trend was reversed until Rosetta was about 670 million km from the Sun when there was once again enough solar energy to power the whole spacecraft.

PictureNews of Rosetta's survival was greeted with some relief at ESOC.
After the OBC delivered the wake-up call at 10.00 UT on 20 January, the attitude control subsystem was brought online to execute a despin manoeuvre and to point the spacecraft’s high gain antenna to Earth to let the mission operators know that the spacecraft had survived hibernation.  The signal was received by NASA’s Deep Space Network antennas at Goldstone California and Canberra Australia at 18.18 UT on the same day, and this was relayed over-ground to Rosetta’s operations team at the European Space Operations Centre (ESOC) in Darmstadt Germany, where news of Rosetta’s survival was received with great relief and celebration.

At wake up, Rosetta still had 9 million km to go to reach Comet 67P/Churnyumov-Gerasimenko, giving operators a few months to check out the spacecraft and its payload instruments.  Rosetta’s first images of the comet are expected in May 2014 from a distance of about 2 million km.  At the end of May, a major course correction manoeuvre will be executed to initiate rendezvous with the target in August.  Release of the lander is scheduled for November 2014.  Watch this space, for Part 4 of this mission review in which we’ll be looking ahead at the rendezvous, orbit and landing phases of the mission.


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    Graham Swinerd - I hope to use this page to highlight current major events in space and spacececraft.

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