Throughout the entire Rosetta mission, the Flight Dynamics team at ESOC have been some of the hardest-working, behind-the-scenes wizards ensuring navigation – and today is no exception. They also have some of the coolest visualization tools in the Solar System!
Flight dynamics team at ESOC
- access_time 30/09/2016
- chat_bubble_outline 7 comments
Written by
Daniel
Daniel Scuka works on the ESA Communication team.
access_time
30 September 2016
chat_bubble_outline
7 comments
format_list_bulleted
Ambition the film
Click image to watch Ambition
Read Rosetta: the ambition to turn science fiction into science fact
Mission milestones
Event | Date |
Launch | 2 Mar 2004 |
Earth swingby | 4 Mar 2005 |
Mars swingby | 25 Feb 2007 |
... more |
Discussion: 7 comments
The screenshot on the left with the red trajectories seems the most interesting for me — I was missing this information from the blog posts. They nicely visualize the Kepler ellipse orbits and how one shifts from one to another one with the manoeuvres (the kink in the lower left ellipse). What kind of shape does the “collision orbit” have?
That ‘collision orbit’ is a free fall towards the comet, so basically a parabola. However, it will be somewhat distorted by the gravitational field of the weirdly formed comet (not exactly a perfect orb…) and any outgassing from the comet Rosetta encounters. The latter is only noticeable because of the very low crash speed (due to the comet’s low mass) combined with Rosetta’s large surface, i.e. solar panels.
It is a hyperbolic trajectory. It has a very high eccentricity, so almost a straight line
Well done, Pablo!! And the rest of the team too!! 🙂
Thanks, Marce,
Congrats to you! Huge your contribution was! 🙂
After browsing through the blog, I found the orbits animations:
https://blogs.esa.int/rosetta/2016/08/05/celebrating-two-years-at-the-comet/
https://blogs.esa.int/rosetta/2016/09/22/rosettas-final-orbits-animation/
[%]D
Gods Speed!