Hubble probes comet 103P/Hartley 2 in preparation for DIXI/EPOXI flyby

Esahubble_opo1035a_1024

esahubble_opo1035a October 5th, 2010

Credit: NASA, ESA, and H. Weaver (The Johns Hopkins University/Applied Physics Lab, USA)

Hubble Space Telescope observations of comet 103P/Hartley 2, taken on 25 September, are helping in the planning for a 4 November flyby of the comet by the Deep Impact eXtended Investigation (DIXI) on NASA's EPOXI spacecraft. Analysis of the new Hubble data shows that the nucleus has a diameter of approximately 1.5 kilometres, which is consistent with previous estimates. The comet is in a highly active state as it approaches the Sun. The Hubble data show that the coma is remarkably uniform, with no evidence for the types of outgassing jets seen from most "Jupiter Family" comets, of which Hartley 2 is a member. Jets can be produced when the dust emanates from a few specific icy regions, while most of the surface is covered with relatively inert, meteoritic-like material. In stark contrast, the activity from Hartley 2's nucleus appears to be more uniformly distributed over its entire surface, perhaps indicating a relatively "young" surface that hasn't yet been crusted over. Hubble's spectrographs the Cosmic Origins Spectrograph (COS) and the Space Telescope Imaging Spectrograph (STIS) are expected to provide unique information about the comet's chemical composition that might not be obtainable any other way, including measurements by DIXI. The Hubble team is specifically searching for emissions from carbon monoxide (CO) and diatomic sulfur (S2). These molecules have been seen in other comets but have not yet been detected in 103P/Hartley 2. 103P/Hartley has an orbital period of 6.46 years. It was discovered by Malcolm Hartley in 1986 at the Schmidt Telescope Unit in Siding Spring, Australia. The comet will pass within 18 million kilometres of Earth (about 45 times the distance to the Moon) on 20 October. During that time the comet may be visible to the naked eye as a 5th magnitude "fuzzy star" in the constellation Auriga.

Provider: Hubble Space Telescope | ESA

Image Source: https://www.spacetelescope.org/images/opo1035a/

Curator: ESA/Hubble, Garching bei München, Germany

Image Use Policy: Creative Commons Attribution 4.0 International License

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Image Details Image Details

Image Type
Observation
Object Name
103P/Hartley 2
Subject - Solar System
Interplanetary Body > Comet

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (STIS ) Optical (V) 550.0 nm
Spectrum_base
Blue
Esahubble_opo1035a_1280
×
ID
opo1035a
Subject Category
A.2.2  
Subject Name
103P/Hartley 2
Credits
NASA, ESA, and H. Weaver (The Johns Hopkins University/Applied Physics Lab, USA)
Release Date
2010-10-05T21:00:00
Lightyears
Redshift
Reference Url
https://www.spacetelescope.org/images/opo1035a/
Type
Observation
Image Quality
Distance Notes
N/A
Facility
Hubble Space Telescope
Instrument
STIS
Color Assignment
Blue
Band
Optical
Bandpass
V
Central Wavelength
550
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
Equinox
Reference Value
Reference Dimension
Reference Pixel
Scale
Rotation
Coordinate System Projection:
Quality
FITS Header
Notes
Creator (Curator)
ESA/Hubble
URL
http://www.spacetelescope.org/
Name
Email
Telephone
Address
Karl-Schwarzschild-Strasse 2
City
Garching bei München
State/Province
Postal Code
D-85748
Country
Germany
Rights
Creative Commons Attribution 4.0 International License
Publisher
ESA/Hubble
Publisher ID
esahubble
Resource ID
opo1035a
Metadata Date
2019-10-07T11:41:39.095528
Metadata Version
1.1
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Detailed color mapping information coming soon...

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There is no distance meta data in this image.

 

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