Asset Details
MbrlCatalogueTitleDetail
Do you wish to reserve the book?
Comet McNaught (260P/2012 K2): spin axis orientation and rotation period
by
Mobberley, Martin
, Oldani, Virginio
, Borrero, José
, Crippa, Roberto
, Nicolas, Joel
, Bryssink, Erik
, Manzini, Federico
in
Astrobiology
/ Astronomy
/ Astrophysics
/ Astrophysics and Astroparticles
/ Comets
/ Cosmology
/ Observations and Techniques
/ Original Article
/ Physics
/ Physics and Astronomy
/ Space Exploration and Astronautics
/ Space Sciences (including Extraterrestrial Physics
2014
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
You are currently in the queue to collect this book. You will be notified once it is your turn to collect the book.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
Comet McNaught (260P/2012 K2): spin axis orientation and rotation period
by
Mobberley, Martin
, Oldani, Virginio
, Borrero, José
, Crippa, Roberto
, Nicolas, Joel
, Bryssink, Erik
, Manzini, Federico
in
Astrobiology
/ Astronomy
/ Astrophysics
/ Astrophysics and Astroparticles
/ Comets
/ Cosmology
/ Observations and Techniques
/ Original Article
/ Physics
/ Physics and Astronomy
/ Space Exploration and Astronautics
/ Space Sciences (including Extraterrestrial Physics
2014
Oops! Something went wrong.
While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
Comet McNaught (260P/2012 K2): spin axis orientation and rotation period
by
Mobberley, Martin
, Oldani, Virginio
, Borrero, José
, Crippa, Roberto
, Nicolas, Joel
, Bryssink, Erik
, Manzini, Federico
in
Astrobiology
/ Astronomy
/ Astrophysics
/ Astrophysics and Astroparticles
/ Comets
/ Cosmology
/ Observations and Techniques
/ Original Article
/ Physics
/ Physics and Astronomy
/ Space Exploration and Astronautics
/ Space Sciences (including Extraterrestrial Physics
2014
Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
Comet McNaught (260P/2012 K2): spin axis orientation and rotation period
Journal Article
Comet McNaught (260P/2012 K2): spin axis orientation and rotation period
2014
Request Book From Autostore
and Choose the Collection Method
Overview
Extensive observations of comet 260P/McNaught were carried out between August 2012 and January 2013. The images obtained were used to analyze the comet’s inner coma morphology at resolutions ranging from 250 to about 1000 km/pixel.
A deep investigation of the dust features in the inner coma allowed us to identify only a single main active source on the comet’s nucleus, at an estimated latitude of −50
∘
±15
∘
.
A thorough analysis of the appearance and of the motion of the morphological structures, supported by graphic simulations of the geometrical conditions of the observations, allowed us to determine a pole orientation located within a circular spot of a 15
∘
-radius centered at RA=60
∘
, Dec=0
∘
. The rotation of the nucleus seems to occur on a single axis and is not chaotic, furthermore no precession effects could be estimated from our measurements.
The comet’s spin axis never reached the plane of the sky from October 2012 to January 2013; during this period it did not change its direction significantly (less than 30
∘
), thus giving us the opportunity to observe mainly structures such as bow-shaped jets departing from the single active source located on the comet’s nucleus.
Only during the months of August 2012 and January 2013 the polar axis was directed towards the Earth at an angle of about 45
∘
from the plane of the sky; this made it possible to observe the development of faint structures like fragments of shells or spirals.
A possible rotation period of 0.340±0.01 days was estimated by means of differential photometric analysis.
Publisher
Springer Netherlands,Springer Nature B.V
MBRLCatalogueRelatedBooks
Related Items
Related Items
We currently cannot retrieve any items related to this title. Kindly check back at a later time.
This website uses cookies to ensure you get the best experience on our website.