ESA still searching for Philae; may have zeroed in on a possible location

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The European Space Agency (ESA) hasn’t given up on the task of finding its Philae comet lander and according to the latest information from the space agency, it may have zeroed in on Philae’s location as being the CONSERT ellipse measuring approximately 16 x 160 m.

Post its landing on the comet 67P/Churyumov-Gerasimenko, the Phiale was operational for 60 hours after which it went silent owing to lack of power. The lander’s batteries would have charged if the lander would have landed in the predesignated spot. However, Philae’s harpoons did not deploy and the ice screws alone proved insufficient to secure the lander at Agilkia. As a result, the lander rebounded for an additional two-hour flight before finally coming to rest at a site now known as Abydos.

This means that Philae’s panel may not have opened up properly to receive enough sunlight to charge its batteries or it may have landed in a place where there is partial or no sunlight.

Alongside Rosetta’s main scientific mission, the spacecraft orbiting the comet has been employed to take closeup images of the possible landing sites.

The highest resolution images taken of the region of interest after Philae’s landing were part of a dedicated search that took place in mid-December, at distance of roughly 18 kilometres from the surface of the comet, notes the space agency. At this distance, the OSIRIS narrow-angle camera has a resolution of 34 centimetres per pixel. The body of Philae is just 1 metre across, while its three thin legs extend out by up to 1.4 metres from its centre.

Taking into account the size, reflectivity, and orientation of Philae, along with the ‘point spread function’ or intrinsic resolution of the camera optics, the OSIRIS team expect Philae to be no more than a few pixels across in their images. Their examination of the head of Comet 67P/C-G revealed many initial candidates for Philae in the form of bright spots just a few pixels wide, as illustrated in the montage below:

Credits: Centre image: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0; insets: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

Credits: Centre image: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0; insets: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

ESA says in its latest update that scientists were able to narrow down the lander’s final location by using the radio signals sent between Philae and Rosetta as part of the CONSERT experiment after the final touchdown.

Combining data on the signal travel time between the two spacecraft with the known trajectory of Rosetta and the current best shape model for the comet, the CONSERT team have been able to establish the location of Philae to within an ellipse roughly 16 x 160 metres in size, just outside the rim of the Hatmehit depression.

Credits: ESA/Rosetta/Philae/CONSERT

Credits: ESA/Rosetta/Philae/CONSERT

According to ESA, the team looking for Philae has narrowed down to the ellipse which is the current best estimate of the outer bounds of the likely location of Philae based on a number of simulations, but further work is being carried out to quantify things more rigorously in terms of the statistical likelihood of Philae being inside this region. The location of the ellipse also depends on the assumed shape model of the comet: as this is constantly being refined, some slight revisions in the positioning of the ellipse remain possible.

“We have identified several possible lander candidates in OSIRIS images, both inside the CONSERT region of interest and nearby,” says Holger Sierks, OSIRIS principal investigator at the Max Planck Institute for Solar System Research (MPS) in Germany.

Holger adds: “That said, it is important to note that the viewing geometry during our December search was such that Rosetta was 90 degrees to the Sun-comet direction and in a terminator orbit. Philae’s solar panels could have been well illuminated, but still hidden in the rugged terrain from Rosetta’s perspective, making it difficult or impossible to spot.”

Furthermore, and as the image above shows, bright features are common on the surface of the nucleus. The challenge of identifying Philae is made even more difficult by the fact that many of them are transient. For example, small-scale regions of the nucleus may “glint” under favourable illumination conditions, thus appearing in some images but not others.

To address this issue, scientists working with OSIRIS team member Philippe Lamy at the Laboratoire d’Astrophysique de Marseille (LAM) and the Institut de Recherche en Astrophysique et Planétologie (IRAP) in France began searching for special sets of OSIRIS images.

In particular, they looked for images taken before and after Philae’s landing under nearly similar illumination conditions, to reduce the chances of being fooled by transient surface features glinting. In that way, if something new appeared after landing, it could be Philae.



The ‘after’ images have been resampled and interpolated to be on the same scale as the ‘before’ image: this results in the bright spot covering more pixels than in the original data.

“Although the pre- and post-landing images were taken at different spatial resolutions, local topographic details match well, except for one bright spot present on post-landing images, which we suggest is a good candidate for the lander,” says Philippe Lamy, member of the OSIRIS team at the Laboratoire d’Astrophysique de Marseille, adding: “This bright spot is visible on two different images taken in December 2014, clearly indicating that it is a real feature on the surface of the comet, not a detector artefact or moving foreground dust speck.”

But is this really Philae? Unfortunately, it is impossible to be sure.

On one hand, analyses carried out at the Philae Science Operations and Navigation Center (SONC) at CNES suggest that this candidate satisfies a number of constraints regarding, for example, illumination and radio visibility in this region.

On the other, the candidate is located just outside the ellipse currently identified by CONSERT, although as mentioned earlier, improved shape models and continued CONSERT data analysis may alter its position.

Also, given the relatively long seven week interval between the ‘before’ and ‘after’ images, it is possible that this object is due to a physical change at that location on the nucleus, perhaps as fresher material was newly exposed. The relative lack of significant illumination in this region at the time argues that such changes are unlikely, but they cannot be completely ruled out.

Ultimately, a definitive identification of this or any other candidate as being Philae will require higher-resolution imaging, in turn meaning closer flybys. This may not be possible in the near-term, as issues encountered in navigating close to the comet mean that the opportunity to make flybys at significantly less than 20 km from the surface may be on hold until later in the mission. But after the comet’s activity has subsided, Rosetta should be able to safely operate in close proximity to the comet nucleus again.

The other possibility of further refining Philae’s location would come if the lander were to receive enough power to wake-up from its hibernation and resume its scientific study of 67P/C-G. Then, CONSERT could be used to perform additional ranging measurements and significantly reduce the uncertainties on the lander’s location.

At the moment, Philae is still in hibernation, but the mission team remain hopeful that, as the comet moves closer to the Sun along its orbit, the lander will receive enough power in the coming weeks or months to wake up and transmit a signal to Rosetta.

“The conditions for Philae’s wake-up are becoming more and more favourable as the comet approaches the Sun,” says Lander Project Manager Stephan Ulamec. “The team at DLR’s Lander Control Center has continued to prepare long term operations for Philae and its instruments in the hope that it does wake up soon.”

In the meantime, the team continue to search through all available data. Patrick Martin, ESA’s Rosetta mission manager says: “Follow-up work, such as the identification of candidates in other images taken from 20 km or less, along with improved reconstruction of the local topography, may help further narrow down the location of Philae.”

Matt Taylor, ESA’s Rosetta project scientist, adds: “Accurately locating the lander is of great scientific value, in particular for the joint orbiter and lander CONSERT experiment to get the best assessment of the interior structure of the comet nucleus. Knowing where Philae is would provide important context for the lander measurements and valuable information for its possible future operation. In the meantime, Rosetta is continuing to observe the comet from a range of distances as the comet’s activity increases.”