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Hot Topic Solar System Meteorites, Comets and Asteroids Rosetta Should Look South for a Landing Site
 
Rosetta Should Look South for a Landing Site
Based on a European Planetary Science Congress news release
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Meteorites, Comets and Asteroids
Posted:   09/26/10

Summary: Scientists have determined that ESA's Rosetta mission needs to deliver its lander to a site in the southern hemisphere of comet 67P/Churyumov-Gerasimenko. A site in this region will be the safest and most scientifically interesting according to the recent study.


Image showing the orbit of comet Churyumov-Gerasimenko and Rosetta during the encounter (not to scale). Credit: ESA
ESA’s Rosetta mission needs to deliver its lander, Philae, to a site in the southern hemisphere of comet 67P/Churyumov-Gerasimenko, according to a new study of the comet’s nucleus.

“Southern sites appear to be both the safest and the most scientifically interesting,” said Jeremie Lasue, who presented the findings at the European Planetary Science Congress in Rome on Thursday 23rd September.

“Churyumov-Gerasimenko is a time capsule holding material from the birth of the Solar System. The nucleus’s southern hemisphere has been heavily eroded, so Philae will not have to drill down far to find those pristine samples. At the time of Rosetta’s rendezvous, gas will be escaping mainly from the northern hemisphere, so it will be safer for Philae to touch down in the south. In addition due to the orientation of the comet, the southern hemisphere will be protected from extreme temperature variations at the time of delivery,” said Lasue.

After a ten-year chase, Rosetta is due to begin maneuvers to rendezvous with comet Churyumov-Gerasimenko in May 2014 and go into orbit around the nucleus in August. Philae is scheduled to drop down onto the surface of the nucleus in November.
Surface illumination of the nucleus of comet Churyumov-Gerasimenko at the time of Rosetta’s rendezvous with the comet at approximately 3.5 AU from the Sun (1 AU = 149.6 million kilometers). The comet nucleus’s rotational period is approximately 12 hours. Credit: Lasue/INAF
The orbiter and lander will then monitor the comet’s evolution over the next 13 months as it approaches the Sun and then travels away again.

Lasue and colleagues from the INAF-IASF and IFSI institutes in Rome have developed three-dimensional computer models that predict the activity of Churyumov-Gerasimenko’s nucleus from the first few months of Rosetta’s initial encounter until the comet’s closest approach in August 2015. Comet nuclei are a porous mixture of dust, ice and frozen gases such as carbon dioxide and carbon monoxide. As the nucleus approaches the Sun and starts to heat up, the gases vaporize and the tail, or coma, starts to form.

The models predict how heat is transferred through the layered nucleus and the vaporization rates of the ices as the comet approaches the Sun. Churyumov-Gerasimenko’s lumpy, diamond-shaped nucleus is tilted at an angle of 45 degrees, which means that the south pole is in the full glare of the Sun at the closest approach. The simulations show that after several orbits close to the Sun, the south pole has been significantly more eroded than the north, potentially giving Philae easy access to pristine cometary material just below the surface. Philae will be able to drill down up to 30 centimeters to collect samples of the cometary soil for on-board analysis.

Surface illumination of the nucleus of comet Churyumov-Gerasimenko at closest approach to the Sun (approximately 1.5 AU). Credit: Lasue/ESA
The south also looks to offer the most stable landing conditions. At the time of landing, the northern hemisphere is illuminated and activity due to escaping gas is concentrated there, with up to 30 kg of gas and 50 kg of dust emitted per second. Gas escaping from the comet’s interior drags dust grains up to the surfaces. Small dust particles are carried away into the coma, while larger grains build up on the surface, forming a coating known as a dust mantle. The simulations show that a dust mantle approximately 20 centimeters deep will have formed in the southern hemisphere, compared to a coating of just a couple of centimeters in northern regions.

“When Philae lands, temperatures at the equator may rise above freezing and could fluctuate by around 150 degrees Celsius. However, the regions close to the south pole will keep more stable temperatures. From our present results, we’ve concluded that the southern hemisphere promises the best landing sites. As more data on Churyumov-Gerasimenko becomes available to better quantify our results, we will be able to add to the picture and help prepare for a safe landing for Philae,” said Maria Cristina De Sanctis, co-author of the study.

Another reason for choosing a southern hemisphere landing site is that Philae is powered by solar cells, so will experience higher levels of illumination as the comet approaches the Sun.

By studying materials from the comet, Philae will help astrobiologists understand if comet impacts on the early Earth could have delivered molecules essential for the origin of life on our planet. Comets can also provide information about the history and evolution of the Solar System - shedding light on how systems that are capable of supporting habitable worlds form.


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