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Deep Impact, Stardust-NExT and the behavior of Comet 9P/Tempel 1 from 1997 to 2010

Meech, K.J., Pittichová, J., Yang, B., Zenn, A., Belton, M.J.S., A'Hearn, M.F., Bagnulo, S., Bai, J., Barrera, L., Bauer, J.M., and others. (2011) Deep Impact, Stardust-NExT and the behavior of Comet 9P/Tempel 1 from 1997 to 2010. Icarus, 213 (1). pp. 323-344. ISSN 0019-1035. (doi:10.1016/j.icarus.2011.02.016) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:52287)

The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided.
Official URL:
http://dx.doi.org/10.1016/j.icarus.2011.02.016

Abstract

We present observational data for Comet 9P/Tempel 1 taken from 1997 through 2010 in an international collaboration in support of the Deep Impact and Stardust-NExT missions. The data were obtained to characterize the nucleus prior to the Deep Impact 2005 encounter, and to enable us to understand the rotation state in order to make a time of arrival adjustment in February 2010 that would allow us to image at least 25% of the nucleus seen by the Deep Impact spacecraft to better than 80m/pixel, and to image the crater made during the encounter, if possible. In total, ~500 whole or partial nights were allocated to this project at 14 observatories worldwide, utilizing 25 telescopes. Seventy percent of these nights yielded useful data. The data were used to determine the linear phase coefficient for the comet in the R-band to be 0.045±0.001magdeg -1 from 1° to 16°. Cometary activity was observed to begin inbound near r~4.0 AU and the activity ended near r~4.6 AU as seen from the heliocentric secular light curves, water-sublimation models and from dust dynamical modeling. The light curve exhibits a significant pre- and post-perihelion brightness and activity asymmetry. There was a secular decrease in activity between the 2000 and 2005 perihelion passages of ~20%. The post-perihelion light curve cannot be easily explained by a simple decrease in solar insolation or observing geometry. CN emission was detected in the comet at 2.43 AU pre-perihelion, and by r=2.24 AU emission from C 2 and C 3 were evident. In December 2004 the production rate of CN increased from 1.8×10 23mols -1 to Q CN=2.75×10 23mols -1 in early January 2005 and 9.3×10 24mols -1 on June 6, 2005 at r=1.53 AU. © 2011 Elsevier Inc.

Item Type: Article
DOI/Identification number: 10.1016/j.icarus.2011.02.016
Additional information: Unmapped bibliographic data: LA - English [Field not mapped to EPrints] J2 - Icarus [Field not mapped to EPrints] AD - Univ. Hawai'i, Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, United States [Field not mapped to EPrints] AD - Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, United States [Field not mapped to EPrints] AD - Belton Space Exploration Initiatives, LLC, 430 S. Randolph Way, Tucson, AZ 85716, United States [Field not mapped to EPrints] AD - Univ. Maryland, Dept. of Astronomy, College Park, MD 20742, United States [Field not mapped to EPrints] AD - Armagh Observatory, College Hill, Armagh BT61 9DG, United Kingdom [Field not mapped to EPrints] AD - Yunnan Astronomical Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 65011, Yunnan, China [Field not mapped to EPrints] AD - Universidad Metropolitana de Ciencias de la Educacíon, Dep. Fisica, Avda. Jose Pedro Alessandri 774, Santiago, Chile [Field not mapped to EPrints] AD - Jet Propulsion Laboratory, MS 183-301, 4800 Oak Grove Drive, Pasadena, CA 91109, United States [Field not mapped to EPrints] AD - University of Hawai'i, Honolulu, HI 96822, United States [Field not mapped to EPrints] AD - Indian Institute of Astrophysics, II Block, Koramangala, Bangalore 560 034, India [Field not mapped to EPrints] AD - Max-Planck Institut fur Sonnensystemforschung, Max-Planck Str. 2, 37191 Katlenburg-Lindau, Germany [Field not mapped to EPrints] AD - The Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, 69978 Tel-Aviv, Israel [Field not mapped to EPrints] AD - Southwest Research Institute, 1050 Walnut St., Suite 300, Boulder, CO 80302, United States [Field not mapped to EPrints] AD - Geminit Observatory, C/o AURA, Casilla 603, La Serena, Chile [Field not mapped to EPrints] AD - Grad. Inst. of Astronomy, National Central Univ., 300 Jhongda Road, Jhongli 32001, Taiwan [Field not mapped to EPrints] AD - Jet Propulsion Laboratory, MS 301-150, 4800 Oak Grove Drive, Pasadena, CA 91109, United States [Field not mapped to EPrints] AD - National Central University, Jhongli City 320, Taiwan [Field not mapped to EPrints] AD - Korea Astronomy and Space Science Institute, 776 Daedukdaero, Yuseong-gu, Daejeon 305-348, South Korea [Field not mapped to EPrints] AD - Univ. Texas, Dept. Astronomy, 1 University Station, C1400, Austin, TX 78712, United States [Field not mapped to EPrints] AD - Centre for Astrophysics and Planetary Science, School of Physical Sciences, The University of Kent, Canterbury CT2 7NH, United Kingdom [Field not mapped to EPrints] AD - Univ. Central Florida, Dept. of Physics, 4000 Central Florida Blvd., Orlando, FL 32816-2385, United States [Field not mapped to EPrints] AD - Instituto de Astrofísica de Andalucía, CSIC, Camino Bajo de Huétor 50, 18080 Granada, Spain [Field not mapped to EPrints] AD - European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching bei Munchen, Germany [Field not mapped to EPrints] AD - Geophysical Institute, Univ. AK, 903 Koyukuk Dr., Fairbanks, AK 99775-7320, United States [Field not mapped to EPrints] AD - Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001, United States [Field not mapped to EPrints] AD - Yonsei University, Dept. of Astronomy, 134 Sinchon-dong, Seodaemun-gu, Seoul 120-749, South Korea [Field not mapped to EPrints] AD - Dept. of Physics and Astronomy, Texas A and M Univ., College Station, TX 77843-4242, United States [Field not mapped to EPrints] AD - National Optical Astronomy Observatory, 950 N. Cherry Ave., Tucson, AZ 85719, United States [Field not mapped to EPrints] AD - Instituto de Astrofísica de Canarias, Dept. de Astrofísica, Universidad de La Laguna, C/Vía Láctea s/n, E-38205 La Laguna, Tenerife, Spain [Field not mapped to EPrints] AD - Goddard Spaceflight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, United States [Field not mapped to EPrints] AD - Dept. of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Rd., Washington, DC 20015, United States [Field not mapped to EPrints] AD - Planetary Science Institute, 1700 E. Ft. Lowell Rd., Suite 106, Tucson, AZ 85719, United States [Field not mapped to EPrints] AD - Dept. Geophysics and Planetary Sciences, Tel Aviv University, 69978 Tel-Aviv, Israel [Field not mapped to EPrints] AD - National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka-shi, JP Tokyo 181-8588, Japan [Field not mapped to EPrints] AD - Lowell Observatory and Institute for Astrophysical Research, Boston University, 1400 W. Mars Hill Road, Flagstaff, AZ 86001, United States [Field not mapped to EPrints] AD - INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy [Field not mapped to EPrints] AD - HAS, 47-728 Hui Kelu St. #9, Kaneohe, HI 96744, United States [Field not mapped to EPrints] AD - Purple Mountain Obs., Chinese Academy of Sciences, 2# West Beijing Road, Nanjing 210008, China [Field not mapped to EPrints] AD - NASA Astrobiology Institute, United States [Field not mapped to EPrints] AD - Astronomical Institute of Slovak Academy of Sciences, Dúbravská cesta 9, 845 04 Bratislava, Slovakia [Field not mapped to EPrints] DB - Scopus [Field not mapped to EPrints]
Uncontrolled keywords: Comet Tempel 1, Comets, Dust, Comets, Nucleus, Ices, Photometry
Subjects: Q Science > QB Astronomy
Divisions: Divisions > Division of Natural Sciences > Physics and Astronomy
Depositing User: Stephen Lowry
Date Deposited: 08 Dec 2015 22:04 UTC
Last Modified: 16 Nov 2021 10:21 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/52287 (The current URI for this page, for reference purposes)

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