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相关论文: The impact and rotational lightcurves of Comet 9P/…

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We report high-spectral resolution observations of comet 9P/Tempel 1 before, during and after the impact on 4 July 2005 UT of the Deep Impact spacecraft with the comet. These observations were obtained with the HIRES instrument on Keck 1.…

天体物理学 · 物理学 2009-11-11 Anita L. Cochran , William M. Jackson , Karen J. Meech , Micah Glaz

We have obtained optical spectrophotometry of the evolution of comet 9P/Tempel 1 after the impact of the Deep Impact probe, using the Supernova Integral Field Spectrograph (SNIFS) at the UH 2.2m telescope, as well as simultaneous optical…

The time dependence of the changes in the emission spectra of Comet 9P/Tempel 1 after Deep Impact are derived and discussed. This was a unique event because for the first time it gave astronomers the opportunity to follow the time history…

地球与行星天体物理 · 物理学 2011-02-11 William M. Jackson , XueLiang Yang , Xiaoyu Shi , Anita L. Cochran

High resolution spectropolarimetry of the Deep Impact target, comet 9P/ Tempel 1, was performed during the impact event on July 4th, 2005 with the HiVIS Spectropolarimeter and the AEOS 3.67m telescope on Haleakala, Maui. We observed…

天体物理学 · 物理学 2009-11-11 D. M. Harrington , K. Meech , L. Kolokolova , J. R. Kuhn , K. Whitman

We have been modeling the envelope of the secular light curve (Ferr\'in, 2010) of comet 1P/Halley. As the first step we have modeled the water production rate of the comet, for several active regions as a function of visual albedo and…

地球与行星天体物理 · 物理学 2011-04-01 Eduardo Rondón , Ignacio Ferrín

One of the least understood properties of comets is the compositional structure of their nuclei, which can either be homogeneous or heterogeneous. The nucleus structure can be conveniently studied at millimeter wavelengths, using…

地球与行星天体物理 · 物理学 2015-06-04 Michal Drahus , David Jewitt , Aurelie Guilbert-Lepoutre , Waclaw Waniak , Albrecht Sievers

We analyzed Deep Impact High Resolution Instrument (HRI) images acquired within the first seconds after collision of the Deep Impact impactor with the nucleus of comet 9P/Tempel 1. These images reveal an optically thick ejecta plume that…

地球与行星天体物理 · 物理学 2014-06-13 Lev Nagdimunov , Ludmilla Kolokolova , Michael Wolff , Michael F. A'Hearn , Tony L. Farnham

GALEX observations of comet 9P/Tempel 1 using the near ultraviolet (NUV) objective grism were made before, during and after the Deep Impact event that occurred on 2005 July 4 at 05:52:03 UT when a 370 kg NASA spacecraft was maneuvered into…

Observing the vibrational/rotational lines in a comet's optical spectrum requires high-resolution spectroscopy, as they are otherwise seen as a blended feature. To achieve this, we have obtained medium and high-resolution (R…

地球与行星天体物理 · 物理学 2024-04-11 K Aravind , Kumar Venkataramani , Shashikiran Ganesh , Arun Surya , Thirupathi Sivarani , Devendra Sahu , Athira Unni , Anil Bhardwaj

We report on the Hubble Space Telescope program to observe periodic comet 9P/Tempel 1 in conjunction with NASA's Deep Impact mission. Our objectives were to study the generation and evolution of the coma resulting from the impact and to…

We use a quasi 3-D thermal evolution model for a spherical comet nucleus, which takes into account the diurnal and latitudinal variation of the solar flux, but neglects lateral heat conduction. We model the thermal evolution and activity of…

天体物理学 · 物理学 2009-11-11 G. Sarid , D. Prialnik , K. J. Meech , J. Pittichova , T. L. Farnham

We report on observations of comet 9P/Tempel 1 carried out before, during, and after the NASA DEEP IMPACT event (UT July 4), with the optical spectrometers UVES and HIRES mounted on the telescopes Kueyen of the ESO VLT (Chile) and Keck 1 on…

We report on low-spectral resolution observations of comet 9P/Tempel 1 from 1983, 1989, 1994 and 2005 using the 2.7m Harlan J. Smith telescope of McDonald Observatory. This comet was the target of NASA's Deep Impact mission and our…

天体物理学 · 物理学 2009-11-13 Anita L. Cochran , Edwin S. Barker , Marcos D. Caballero , Judit Gyorgey-Ries

The 4050\AA\ band of C$_3$ was observed with Keck/HIRES echelle spectrometer during the {\em Deep Impact} encounter. We perform a 2-dimensional analysis of the exposures in order to study the spatial, spectral, and temporal changes in the…

地球与行星天体物理 · 物理学 2015-06-05 Máté Ádámkovics , Imke de Pater , Hy Spinrad

The nuclei of active comets emit molecules anisotropically from discrete vents. As the nucleus rotates, we expect to observe periodic variability in the molecular emission line profiles, which can be studied through mm/submm spectroscopy.…

Spectropolarimetry of the Deep Impact target, comet 9P/ Tempel 1, was performed during the impact event on July 4th, 2005 with the HiVIS Spectropolarimeter and the AEOS 3.67m telescope on Haleakala, Maui. We observed atypical polarization…

天体物理学 · 物理学 2015-06-24 D. M. Harrington , K. Meech , L. Kolokolova , J. R. Kuhn , K. Whitman

We present results from an atmospheric circulation study of nine hot Jupiters that comprise a large transmission spectral survey using the Hubble and Spitzer Space Telescopes. These observations exhibit a range of spectral behavior over…

地球与行星天体物理 · 物理学 2016-04-20 Tiffany Kataria , David K. Sing , Nikole K. Lewis , Channon Visscher , Adam P. Showman , Jonathan J. Fortney , Mark S. Marley

We present an attempt to extract information about the comet 9P/Tempel 1 nucleus from the characteristics of the ejecta cloud produced by the impactor of the Deep Impact mission. For this purpose we use two techniques. We first study the…

地球与行星天体物理 · 物理学 2016-12-07 Ludmilla Kolokolova , Lev Nagdimunov , Michael A`Hearn , Ashley King , Michael Wolff

We present new analyses of the photometric lightcurve of Comet 1P/Halley during its 1985/86 apparition. As part of a world-wide campaign coordinated by the International Halley Watch (IHW), narrowband photometry was obtained with telescopes…

We report on spectroscopic observations of periodic comet 9P/Tempel 1 by the Alice ultraviolet spectrograph on the Rosetta spacecraft in conjunction with NASA's Deep Impact mission. Our objectives were to measure an increase in atomic and…

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