Rosetta. The end of the mission.

 

 
Artist's impression of Rosetta shortly before hitting Comet 67P/Churyumov–Gerasimenko on 30 September 2016. 
Credit: ESA/ATG medialab 
 

After more than 12 years in space, and two years following comet 67P/Churyumov–Gerasimenko as they orbited the Sun, Rosetta mission concluded on September 30, 2016 with the spacecraft descending onto the comet in a region hosting several ancient pits.

   Rosetta was a European Space Agency (ESA) mission with contributions from its member states and NASA. Rosetta’s Philae lander was provided by a consortium led by DLR, MPS, CNES and ASI. Since launch in 2004, Rosetta was in its sixth orbit around the Sun. Its nearly 8 billion-kilometre journey included three Earth flybys and one at Mars, and two asteroid encounters. The craft endured 31 months in deep-space hibernation on the most distant leg of its journey, before waking up in January 2014 and finally arriving at the comet in August 2014. After becoming the first spacecraft to orbit a comet, and the first to deploy a lander, Philae, in November 2014, Rosetta continued to monitor the comet’s evolution during their closest approach to the Sun and beyond. 

   The decision to end the mission was predicated on the fact that the comet was heading out beyond the orbit of Jupiter, and there would be little power to operate the spacecraft. The date selected for the end of mission was immediately before entering superior solar conjunction, when the Sun is close to the line-of-sight between Earth and Rosetta, meaning communications with the craft would have become increasingly more difficult. 

 
  A colour image of Comet 67P/Churyumov-Gerasimenko composed of three images taken by Rosetta's scientific imaging system OSIRIS in the red, green and blue filters. The images were taken on 6 August 2014 from a distance of 120 kilometres from the comet. Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA
 
Rosetta’s trajectory from the last flyover to controlled descent, as seen from Sun (top) and close to the terminator plane (bottom)
 

 

   The spacecraft began a 19 kilometers descent with a 208-second thruster burn executed on September 19, 2016, at approximately 20:50 UTC. During the descent, Rosetta studied the comet’s gas, dust, and plasma environment very close to the surface and took numerous high-resolution images. Rosetta was targeting a point within a 700 x 500 metre ellipse, between two pits in the Ma’at region, on the comet's smaller lobe. Reconstruction of the final descent trajectory showed that the spacecraft touched down at 10:39:34 UTC at the comet, 26 seconds earlier than the target time, and only 33 metres away from the target, some 720 million km from Earth. Rosetta’s signal disappeared from screens at ESA’s mission control at 11:19:37 UT. The touchdown site was subsequently named Sais after a town in Egypt where the Rosetta Stone, for which the mission was named, is thought to have been originally located.

   No large dust particles were collected during the descent. The final image, reconstructed after Rosetta’s landing, was taken with the OSIRIS wide-angle camera at an altitude of about 20 metres above the impact point and had a scale of 2 mm/pixel. Prior to that, much of the imaging campaign during the descent focused on the 130 metre-wide pit named Deir el-Medina. The camera succeeded in capturing detailed images of the inside of the pit and its walls. These images will be used to help understand the comet’s subsurface and thus its geological history.

   Right before impact, one of Rosetta’s star trackers generated an event reporting a ‘Large Object’ in the field of view: this was the local comet ‘horizon’. Upon touchdown, the signal coming from Rosetta was lost, and mission operators believe that this was most likely caused by the high gain antenna immediately off-pointing from Earth at impact. No further telemetry was received subsequently, indicating that the planned safe mode and subsequent shut down of the spacecraft likely occurred successfully.

  However, Rosetta's usefulness does not entirely come to an end. Safely preserved beneath the spacecraft's thermal blankets is the Rosetta Disk, the modern equivalent of the original Rosetta Stone. Micro-etched on this 7.5 cm nickel disk are 1000 different languages, a comprehensive cultural archive gathered by the San Francisco-based Long Now Foundation. Each page of text, which is miniaturized and etched onto the disk as an image, requires only a microscope to be read. Such simplicity guards against the threat of changing technologies, which could make a digital disk unreadable by computers in the future. 

 

  
An image taken by the OSIRIS narrow-angle camera from an altitude of 5.7 km, during Rosetta’s descent on 30 September 2016. The image scale is about 11 cm/pixel and the image measures about 225 m across. The final touchdown point, named Sais, is seen in the bottom right of the image and is located within a shallow, ancient pit. Exposed, dust-free terrain is seen in the pit walls and cliff edges. 
Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA 
 
  Rosetta’s OSIRIS wide-angle camera captured this view of Comet 67P/Churyumov–Gerasimenko from a height of 331 m above the surface during its final descent on 30 September 2016. The image scale is about 33 mm/pixel and the image measures about 55 m across. The image shows a mix of coarse and fine-grained material.
Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA  
 
  The final image from Rosetta, shortly before it made a controlled impact onto Comet 67P/Churyumov–Gerasimenko on 30 September 2016, was taken at an altitude of 19.5±1.5 m. It was reconstructed from residual telemetry. The image has a scale of 2 mm/pixel and measures about 1 m across.
Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA
 
 
 
    A compilation of images taken by Rosetta’s high resolution OSIRIS camera during the mission’s final hours at comet 67P/Churyumov-Gerasimenko. As it moved closer towards the surface it scanned across an ancient pit and sent back images showing what would become its final resting place.
Credits: Images: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA
Image compilation: ESA–D. C. Jimeno and M. P. Ayucar.  CC BY-SA 4.0

 

 

References:

ESA: Mission complete: Rosetta’s journey ends in daring descent to comet. 30 September 2016
Pablo Muñoz et al. Rosetta navigation during the end of mission phase [PDF]. Symposium on Space, 2017

 

© 2025, Andrew Mirecki 

 

 


 

 

 

 

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