SwePub
Sök i LIBRIS databas

  Extended search

WFRF:(Agarwal M)
 

Search: WFRF:(Agarwal M) > (2010-2014) > The rotation state ...

The rotation state of 67P/Churyumov-Gerasimenko from approach observations with the OSIRIS cameras on Rosetta

Mottola, S. (author)
Lowry, S. (author)
Snodgrass, C. (author)
show more...
Lamy, P. L. (author)
Toth, I. (author)
Rozek, A. (author)
Sierks, H. (author)
A'Hearn, M. F. (author)
Angrilli, F. (author)
Barbieri, C. (author)
Barucci, M. A. (author)
Bertaux, J-L (author)
Cremonese, G. (author)
Da Deppo, V. (author)
Davidsson, Björn (author)
Uppsala universitet,Institutionen för fysik och astronomi
De Cecco, M. (author)
Debei, S. (author)
Fornasier, S. (author)
Fulle, M. (author)
Groussin, O. (author)
Gutierrez, P. (author)
Hviid, S. F. (author)
Ip, W. (author)
Jorda, L. (author)
Keller, H. U. (author)
Knollenberg, J. (author)
Koschny, D. (author)
Kramm, R. (author)
Kuehrt, E. (author)
Kueppers, M. (author)
Lara, L. (author)
Lazzarin, M. (author)
Lopez Moreno, J. J. (author)
Marzari, F. (author)
Michalik, H. (author)
Naletto, G. (author)
Rickman, Hans (author)
Uppsala universitet,Institutionen för fysik och astronomi
Rodrigo, R. (author)
Sabau, L. (author)
Thomas, N. (author)
Wenzel, K-P (author)
Agarwal, J. (author)
Bertini, I. (author)
Ferri, F. (author)
Guettler, C. (author)
Magrin, S. (author)
Oklay, N. (author)
Tubiana, C. (author)
Vincent, J-B (author)
show less...
 (creator_code:org_t)
2014-09-12
2014
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 569, s. L2-
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Aims. Approach observations with the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) experiment onboard Rosetta are used to determine the rotation period, the direction of the spin axis, and the state of rotation of comet 67P's nucleus. Methods. Photometric time series of 67P have been acquired by OSIRIS since the post wake-up commissioning of the payload in March 2014. Fourier analysis and convex shape inversion methods have been applied to the Rosetta data as well to the available ground-based observations. Results. Evidence is found that the rotation rate of 67P has significantly changed near the time of its 2009 perihelion passage, probably due to sublimation-induced torque. We find that the sidereal rotation periods P-1 = 12.76129 +/- 0.00005 h and P2 = 12.4043 +/- 0.0007 h for the apparitions before and after the 2009 perihelion, respectively, provide the best fit to the observations. No signs of multiple periodicity are found in the light curves down to the noise level, which implies that the comet is presently in a simple rotation state around its axis of largest moment of inertia. We derive a prograde rotation model with spin vector J2000 ecliptic coordinates lambda = 65 degrees +/- 15 degrees, beta = + 59 degrees +/- 15 degrees, corresponding to equatorial coordinates RA = 22 degrees, Dec = +76 degrees. However, we find that the mirror solution, also prograde, at lambda = 275 degrees +/- 15 degrees, beta = + 50 degrees +/- 15 degrees (or RA = 274 degrees, Dec = +27 degrees), is also possible at the same confidence level, due to the intrinsic ambiguity of the photometric problem for observations performed close to the ecliptic plane.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

comets: general
comets: individual: 67P/Churyumov-Gerasimenko
techniques: photometric

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view