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相关论文: Water in the Near IR spectrum of Comet 8P/Tuttle

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We present spectral and spatial information for major volatile species in Comet 10P/Tempel 2, based on high-dispersion infrared spectra acquired on UT 2010 July 26 (heliocentric distance Rh = 1.44 AU) and September 18 (Rh = 1.62 AU),…

地球与行星天体物理 · 物理学 2012-02-10 L. Paganini , M. J. Mumma , B. P. Bonev , G. L. Villanueva , M. A. DiSanti , J. V. Keane , K. J. Meech

We present sensitive 5.5 to 7.6 micron spectra of comet C/2003 K4 (LINEAR) obtained on 16 July 2004 (r_{h} = 1.760 AU, Delta_{Spitzer} = 1.409 AU, phase angle 35.4 degrees) with the Spitzer Space Telescope. The nu_{2} vibrational band of…

天体物理学 · 物理学 2009-11-13 Charles E. Woodward , Michael S. Kelley , Dominique Bockelee-Morvan , R. D. Gehrz

The high spectral resolution and sensitivity of Herschel/HIFI allows for the detection of multiple rotational water lines and accurate determinations of water production rates in comets. In this letter we present HIFI observations of the…

We present results for Chandra observations of comets, 17P/Holmes (17P) and 8P/Tuttle (8P). 17P was observed for 30 ksec right after its major outburst, on 31 Oct 2007 (10:07 UT) and comet 8P/Tuttle was observed in 2008 January for 47 ksec.…

太阳与恒星天体物理 · 物理学 2015-05-18 D. J. Christian , D. Bodewits , C. M. Lisse , K. Dennerl , S. J. Wolk , H. Hsieh , T. H. Zurbuchen , L. Zhao

The recently puplished Barber-Tennyson (BT2) synthetic H$_2$O water line list is the most complete and accurate line list in existence. It is finding application in a wide range of astrophysical environments. UKIRT spectra of comet Tempel…

天体物理学 · 物理学 2007-05-23 R. J. Barber , S. Miller , T. S. Stallard , J. Tennyson

Comet 8P/Tuttle is a Nearly Isotropic Comet (NIC), whose physical properties are poorly known and could be different from those of Ecliptic Comets (EC) owing to their different origin. Two independent observations have shown that 8P has a…

地球与行星天体物理 · 物理学 2019-12-11 O. Groussin , P. L. Lamy , M. S. P. Kelley , I. Toth , L. Jorda , Y. R. Fernández , H. A. Weaver

High-resolution far-infrared and sub-millimetre spectroscopy of water lines is an important tool to understand the physical and chemical properties of cometary atmospheres. We present observations of several rotational ortho- and para-water…

Little is known about the physical properties of cometary nuclei. Apart from space mission targets, measuring the thermal emission of a nucleus is one of the few means to derive its size, independently of its albedo, and to constrain some…

地球与行星天体物理 · 物理学 2015-05-27 J. Boissier , O. Groussin , L. Jorda , P. Lamy , D. Bockelée-Morvan , J. Crovisier , N. Biver , P. Colom , E. Lellouch , R. Moreno

We present 5.5 to 7.6 micron spectra of comets 71P/Clark (2006 May 27.56 UT, r_h = 1.57 AU pre-perihelion) and C/2004 B1 (LINEAR) (2005 October 15.22 UT, r_h = 2.21 AU pre-perihelion and 2006 May 16.22 UT, r_h = 2.06 AU post-perihelion)…

地球与行星天体物理 · 物理学 2010-05-12 Dominique Bockelee-Morvan , Charles E. Woodward , Michael S. Kelley , Diane H. Wooden

We report measurements of eight native (i.e., released directly from the comet nucleus) volatiles (H2O, HCN, CH4, C2H2, C2H6, CO, H2CO, and CH3OH) in comet 8P/Tuttle using NIRSPEC at Keck 2. Comet Tuttle reveals a truly unusual composition,…

天体物理学 · 物理学 2009-11-13 B. P. Bonev , M. J. Mumma , Y. L. Radeva , M. A. DiSanti , E. L. Gibb , G. L. Villanueva

176P/LINEAR is a member of the new cometary class known as main-belt comets (MBCs). It displayed cometary activity shortly during its 2005 perihelion passage that may be driven by the sublimation of sub-surface ices. We have therefore…

On November 4th, 2010, the Deep Impact eXtended Investigation (DIXI) successfully encountered comet 103P/Hartley 2, when it was at a heliocentric distance of 1.06 AU. Spatially resolved near-IR spectra of comet Hartley 2 were acquired in…

Comet 73P-B/Schwassmann-Wachmann 3 was observed with IRCS/Subaru at geocentric distance of 0.074 AU on UT 10 May 2006. Multiple H2O emission lines were detected in non-resonant fluorescence near 2.9 microns. No significant variation in…

We measured organic volatiles (CH4, CH3OH, C2H6, H2CO), CO, and water in comet 8P/Tuttle, a comet from the Oort cloud reservoir now in a short-period Halley-type orbit. We compare its composition with two other comets in Halley-type orbits,…

天体物理学 · 物理学 2010-11-11 H. Boehnhardt , M. J. Mumma , G. L. Villanueva , M. A. DiSanti , B. P. Bonev , M. Lippi , H. U. Kaeufl

On 4 July 2005 at 5:52 UT the Deep Impact mission successfully completed its goal to hit the nucleus of 9P/Tempel 1 with an impactor, forming a crater on the nucleus and ejecting material into the coma of the comet. NASA's Submillimeter…

天体物理学 · 物理学 2009-11-11 F. Bensch , G. J. Melnick , D. A. Neufeld , M. Harwit , R. L. Snell , B. M. Patten , V. Tolls

We present Hubble Space Telescope near-infrared transmission spectroscopy of the transiting hot-Jupiter HAT-P-1b. We observed one transit with Wide Field Camera 3 using the G141 low-resolution grism to cover the wavelength range 1.087-…

The Jupiter-family comet 103P/Hartley 2 (103P) was the target of the NASA EPOXI mission. In support of this mission, we conducted observations from radio to submillimeter wavelengths of comet 103P in the three weeks preceding the spacecraft…

地球与行星天体物理 · 物理学 2015-06-22 A. Gicquel , S. N. Milam , G. L. Villanueva , A. J. Remijan , I. M. Coulson , Y. -L. Chuang , S. B. Charnley , M. A. Cordiner , Y. -J. Kuan

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…

We aimed to measure the H2O and dust production rates in C/2006 W3 (Christensen) with the Herschel Space Observatory at a heliocentric distance of ~ 5 AU. We have searched for emission in the H2O and NH3 ground-state rotational transitions…

Jupiter family comet 17P/Holmes underwent a remarkable outburst on UT 2007 Oct. 24, in which the integrated brightness abruptly increased by about a factor of a million.We obtained near infrared (0.8 - 4.2 micron) spectra of 17P/Holmes on…

地球与行星天体物理 · 物理学 2009-11-13 Bin Yang , David Jewitt , Schelte J. Bus
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