International audienceThe martian upper atmosphere could be strongly perturbed by the near collision with Comet C/2013 A1 (Siding Spring). Significant mass and energy will be deposited in the upper atmosphere of Mars if the comet coma is sufficiently dense. We predict that comet H2O production rates larger than 1028 molecules/s would produce temperature increases exceeding 30 K and the H density in the upper atmosphere will approximately double. The temperature perturbation will persist for several hours and the increased H density for tens of hours. Drag on orbiting spacecraft may increase by substantial factors, depending upon comet activity, because of the thermal perturbation to the atmosphere. Observation of these perturbations may pro...
International audienceOn October 19th 2014, Mars experienced a close encounter with Comet C/2013 A1 ...
We used the Imaging Ultraviolet Spectrograph (IUVS) aboard the Mars Atmosphere and Volatile Evolutio...
International audienceThis paper is a phenomenological description of multi‐spacecraft observations ...
International audienceThe martian upper atmosphere could be strongly perturbed by the near collision...
International audienceOn October 19th 2014, Mars experienced a close encounter with Comet C/2013 A1 ...
The nucleus of comet C/2013 A1 (Siding Spring) passed within 141,000 km of Mars on 19 October 2014. ...
The nucleus of comet C/2013 A1 (Siding Spring) passed within 141,000km of Mars on 19 October 2014. T...
Comet Siding Spring C/2013 A1 will pass Mars on 19 October 2014, entailing particle and dust precipi...
International audienceThe close approach of comet C/2013 A1 (Siding Spring) to Mars in 2014 October ...
International audienceWith the approach of the close encounter of comet Siding Spring with Mars, pos...
International audienceOn October 19th 2014, Mars experienced a close encounter with Comet C/2013 A1 ...
We used the Imaging Ultraviolet Spectrograph (IUVS) aboard the Mars Atmosphere and Volatile Evolutio...
International audienceThis paper is a phenomenological description of multi‐spacecraft observations ...
International audienceThe martian upper atmosphere could be strongly perturbed by the near collision...
International audienceOn October 19th 2014, Mars experienced a close encounter with Comet C/2013 A1 ...
The nucleus of comet C/2013 A1 (Siding Spring) passed within 141,000 km of Mars on 19 October 2014. ...
The nucleus of comet C/2013 A1 (Siding Spring) passed within 141,000km of Mars on 19 October 2014. T...
Comet Siding Spring C/2013 A1 will pass Mars on 19 October 2014, entailing particle and dust precipi...
International audienceThe close approach of comet C/2013 A1 (Siding Spring) to Mars in 2014 October ...
International audienceWith the approach of the close encounter of comet Siding Spring with Mars, pos...
International audienceOn October 19th 2014, Mars experienced a close encounter with Comet C/2013 A1 ...
We used the Imaging Ultraviolet Spectrograph (IUVS) aboard the Mars Atmosphere and Volatile Evolutio...
International audienceThis paper is a phenomenological description of multi‐spacecraft observations ...