Philae wake-up triggers intense planning

Philae wake-up triggers intense planning
This image was taken by Rosetta’s Navigation Camera at 19:38 GMT on 13 June 2015, shortly before Philae’s wake-up signal was received. The signals were relayed by the Rosetta orbiter and received at ESA's European Space Operations Centre in Darmstadt at 20:28 GMT. The image was taken from a distance of 201 km from the centre of Comet 67P/Churyumov-Gerasimenko and measures 17.5 km across. The image scale is 17.1 m/pixel. The comet is orientated with the small lobe towards the right, with the large depression known as Hatmehit visible. Philae is thought to be resting just outside the rim, towards the top right in this image. Credit: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

The receipt of signals from Rosetta's Philae lander on 13 June after 211 days of hibernation marked the start of intense activity. In coordination with its mission partners, ESA teams are working to juggle Rosetta's flight plan to help with renewed lander science investigations.

Philae has woken up after seven months in hibernation on Comet 67P/Churyumov–Gerasimenko. Hidden by shadows, Philae shut down on 15 November 2014 at 00:36 GMT after completing its main sequence on the when the primary battery expired as expected after about 60 hours.

Since March 2015, when Philae's environmental conditions started to improve with higher surface temperatures and better illumination, the orbiter's receiver had been turned on periodically to listen for signals from the when the orbital geometry was thought to be optimum.

On the evening of 13 June, a weak but solid radio link between Rosetta and the lander was finally established for 85 seconds. More than 300 'packets' – 663 kbits – of lander housekeeping telemetry were received. This information had been stored on board at an as-yet-to-be determined time in the past, as much as several days to a few weeks, so does not necessarily reflect the lander's current status.

Rosetta then relayed the signal to ESA's European Space Operations Centre, ESOC, in Darmstadt, Germany, at 20:28 GMT.

Lander subsystems working nominally

"We are still examining the housekeeping information at the Lander Control Centre in the DLR German Aerospace Center's establishment in Cologne, but we can already tell that all lander subsystems are working nominally, with no apparent degradation after more than half a year hiding out on the comet's frozen surface," says DLR's Stephan Ulamec, Philae Lander Project Manager.

A second, smaller burst of lander data was received on Sunday, 14 June, at about 21:26 GMT, lasting just a few seconds. These data were confirmed to give the current status, showing the lander's internal temperature had already risen to –5ºC.

Philae's memory has stored over 8000 packets of additional status data, but it is unclear from when in recent days they were recorded.

Here comes the sun

Engineers at the Lander Control Centre have determined that Philae is already being exposed to sufficient sunlight to heat it to an acceptable operating temperature and to generate electricity.

"Power levels increase during the local 'comet day' – the part of the about-12 hour comet rotation when Philae is in sunlight – from 13 W at comet sunrise to above 24 W," notes ESA's Patrick Martin, Rosetta Mission Manager. "It needs at least 19 W to switch on the transmitter."

Philae wake-up triggers intense planning
Rosetta’s OSIRIS narrow-angle camera witnessed Philae’s descent to the surface of Comet 67P/Churyumov-Gerasimenko yesterday. This animated gif comprises images captured between 10:24 and 14:24 GMT (onboard spacecraft time). More images showing Philae closer to the surface are still to be downloaded. Separation occurred onboard the spacecraft at 08:35 GMT (09:35 CET), with the confirmation signal arriving on Earth at 09:03 GMT (10:03 CET). Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

The telemetry downloaded covered the lander's status for a full night–day cycle of the comet, which is helping ground teams to understand how the Sun is shining on the lander. The solar panels appear to be receiving power for over 135 minutes in each illumination period.

"While the information we have is very preliminary, it appears that the lander is in as good a condition as we could have hoped," says Dr Ulamec.

The task at hand

The main task now for all the mission partners – ESA for Rosetta and DLR and France's CNES space agency for lander operations and science, respectively – is to determine how to optimise Rosetta's orbit so as to facilitate contact and enable new science investigations.

It is believed that there is sufficient power now being generated to allow some science measurements during the time Philae is illuminated, with initial activities focusing on low-power measurements. This first phase would also likely include measurements that did not previously generate science in November.

However, the mission teams first must establish a more robust link between Rosetta and Philae before uploading the first batch of science operations commands.

The quality of the communication link is also possibly related to the trajectory Rosetta is flying and the orientation it adopts.

Optimising an orbit 305 million km away

Currently, Rosetta experiences two possible communication slots per 24 hours – once per 12-hour comet rotation.

Until 23:35 GMT on Tuesday, 16 June, Rosetta will be flying an orbit set by already-uploaded commands on the terminator – the plane between comet day and night – moving out from about 200 km to 235 km altitude.

Philae wake-up triggers intense planning
Rosetta’s lander Philae is safely on the surface of Comet 67P/Churyumov-Gerasimenko, as these first two CIVA images confirm. One of the lander’s three feet can be seen in the foreground. The image is a two-image mosaic. The full panoramic from CIVA will be delivered in this afternoon’s press briefing at 13:00 GMT/14:00 CET. Credit: ESA/Rosetta/Philae/CIVA

This orbit is not optimised for lander communication, so longer periods of contact may not be possible until the trajectory has been changed.

"With work done by the flight dynamics and operations team at ESOC and based on intense planning being conducted with the mission partners today, a new orbit will be devised that ensures optimum lander communications beginning with the next command upload later tonight," says Paolo Ferri, ESA's Head of Mission Operations.

This new orbit will include an already-planned reduction of distance from the nucleus, down to 180 km versus 200 km, and 'nadir pointing' – continuously pointing Rosetta's communications unit at the comet. In the coming days, the orbiter may also be moved closer to the comet, without compromising the safety of the spacecraft, to help communications.

The new orbit will be flown by Rosetta starting after 23:25 GMT on 16 June until 19 June, aiming to enable more and longer contacts with Philae, especially towards the end of this period.

Ready to react quickly

Philae wake-up triggers intense planning
The current 16 x 160 m CONSERT ellipse overlaid on an OSIRIS narrow-angle camera (NAC) image of the same region. The location and size of the ellipse are not accurate at the pixel level, and may also change as further CONSERT data analysis proceeds and more detailed comet shape models become available. The OSIRIS image is a slightly cropped 2 x 2 mosaic of NAC images taken from a distance of approximately 18 km from the surface of the comet on 13 December 2014. At this distance, the resolution of NAC is about 34 cm per pixel, and the full mosaic covers roughly 1.3 km. Ellipse: Credit: ESA/Rosetta/Philae/CONSERT; Image: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

Establishing a regular and predictable pattern of contacts is a prerequisite for performing a complete assessment of the lander's status and for planning science operations.

"If we manage to achieve and maintain a predictable contact pattern," continues Paolo Ferri, "the lander teams can devise a strategy for a new sequence of scientific operations."

"Regardless, we will stay very flexible and be ready to react quickly. It's clear this incredible mission continues to stimulate and challenge us, developing in ways we could never have predicted."

As a bonus, any operation of Philae's instruments up to or through perihelion on 13 August – the comet's closest point to the Sun along its orbit – will allow in-situ study of a comet during its peak activity.

Had Philae landed at the planned site, at Agilkia in November 2014, its mission would likely have ended in March because of the higher temperatures of that location as solar illumination increased.

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