CometWatch 9 October

This image of Comet 67P/Churyumov-Gerasimenko was taken by Rosetta’s NAVCAM on 9 October from a distance of 579 km.

The image scale is 49.4 m/pixel and the image measures 50.5 km across. The contrast is increased to better see the comet’s activity, with several distinct active regions clearly visible.

Single frame enhanced NAVCAM image of Comet 67P/C-G taken on 9 October 2015. Credits: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

Single frame enhanced NAVCAM image of Comet 67P/C-G taken on 9 October 2015. Credits: ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0

In this orientation the comet’s small lobe is in the background, with primarily the Anuket region visible, and the large lobe is in the foreground with parts of Atum, Anubis and Khonsu visible.

Rosetta is currently on its return leg of a 1500 km far excursion to study the wider coma and plasma environment from afar, and is scheduled to reach a distance of 450 km from the comet by tomorrow (Saturday).

 

The original 1024 x 1024 pixel image is provided below.

ESA_Rosetta_NAVCAM_20151009

Comments

10 Comments

  • ianw16 says:

    So that will be ~ 130 km in 8 days. About 16 km per day, or ~ 700 m per hour.. I'm assuming that they will still be looking very closely at the environment through which they are traveling.
    This will add hugely to the results from previous measurements of the environments around comets at Halley, Grigg-Skjellerup and Giacobini-Zinner.
    There is a paper, freely available, on the early results from 67p from 3.6 to 1.2 AU available here: https://iopscience.iop.org/article/10.1088/1742-6596/642/1/012005/meta;jsessionid=703D14177FBD0E156A41FEBE8D119E1E.c1
    In it they compare the results to those obtained at Grigg-Skjellerup, and also to the AMPTE experiment.

    • ianw16 says:

      Sorry, the above paper covers from 3.6 to 1.8 AU.

      • ianw16 says:

        And just in case, to cover myself and the blog mods, under the terms of the Creative Commons 3.0 terms regarding "further distribution" of the paper, I probably should include the following:

        Ion pickup observed at comet 67P with the Rosetta Plasma Consortium (RPC) particle sensors: similarities with previous observations and AMPTE releases, and effects of increasing activity

        Coates, A.J. et al
        IOP Publishing
        Journal of Physics: Conference Series, Vol. 642, No. 1, 2015, pp 12005-12014
        DOI: http://dx.doi.org/10.1088/1742-6596/642/1/012005

        Should be safe now!

        • logan says:

          Thanks Ianw16 🙂

          The deflection part is very important to me [also the electric fields].

  • Sharat says:

    Can we now consider Philae experiment as a lost adventure?

    • emily says:

      Rosetta is still too far from the comet to be in with a good chance of hearing from Philae; once closer again (something like 200 km or less) there will be opportunities again!

  • logan says:

    Jets begin to honor their name. Looking less "auroral".

    Just for remembering:

    http://blogs.esa.int/rosetta/2015/06/19/cometwatch-14-june/

  • Fabian Augustin says:

    Stunning!

  • FCE says:

    Outstanding photos. There is something amazing in this pictures.
    Comet 67P is almost pitch black, reflecting only 6% of incoming light.

  • logan says:

    Are electrons on slow diffusion mode now?

Comments are closed.