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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

We present optical observations and Monte Carlo models of the dust coma, tail, and trail structures of comet 22P/Kopff during the 2002 and 2009 apparitions. Dust loss rates, ejection velocities, and power-law size distribution functions are…

地球与行星天体物理 · 物理学 2015-06-04 Fernando Moreno , Francisco Pozuelos , Francisco Aceituno , Victor Casanova , Alfredo Sota , Julio Castellano , Esteban Reina

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 review the composition of Jupiter-family comet dust as inferred from infrared spectroscopy. We find that Jupiter-family comets have 10 micron silicate emission features with fluxes roughly 20-25% over the dust continuum (emission…

天体物理学 · 物理学 2015-05-13 Michael S. Kelley , Diane H. Wooden

We present the results of imaging photometric and long-slit spectroscopic observations of comet 2P/Encke performed at the heliocentric distance 0.56 au, geocentric distance 0.65 au, and phase angle 109.2 deg on November 4, 2013 and at 1.05…

地球与行星天体物理 · 物理学 2021-01-13 Vera Rosenbush , Oleksandra Ivanova , Valerii Kleshchonok , Nikolai Kiselev , Viktor Afanasiev , Olena Shubina , Dmitry Petrov

Comet 17P/Holmes underwent a massive outburst in 2007 Oct., brightening by a factor of almost a million in under 48 hours. We used infrared images taken by the Wide-Field Survey Explorer mission to characterize the comet as it appeared at a…

地球与行星天体物理 · 物理学 2015-06-19 R. Stevenson , J. M. Bauer , E. A. Kramer , T. Grav , A. K. Mainzer , J. R. Masiero

Comet 7P/Pons-Winnecke was observed from the Calar Alto Observatory (Spain) for four months during the 2021 inbound apparition. Broad-band visible images were taken between 1.71 and 1.25 AU pre-perihelion, while long-slit spectrophotometric…

地球与行星天体物理 · 物理学 2025-03-18 Irene Mariblanca-Escalona , Luisa M. Lara , Fernando Moreno , Pedro J. Gutiérrez , Marçal Evangelista-Santana

We discuss the morphology and spectrophotometry of 5 comets visible in August, 2001. We decompose comae into coma profiles and azimuthally renormalized images, in which general and local features are quantitatively comparable. Comet…

天体物理学 · 物理学 2009-11-07 Gy. M. Szabo , L. L. Kiss , K. Sarneczky , K. Sziladi

We present analyses of Spitzer observations of 29P/Schwassmann-Wachmann 1 using 16 $\mu$m IRS "blue" peak-up (PU) and 24 $\mu$m and 70 $\mu$m MIPS images obtained on UT 2003 November 23 and 24 that characterize the Centaur's large-grain…

We present photometric and morphological analysis of the behavior of sungrazing comet C/2012 S1 ISON in SOHO and STEREO images around its perihelion on 2013 November 28.779 UT. ISON brightened gradually November 20-26 with a superimposed…

地球与行星天体物理 · 物理学 2015-06-18 Matthew M. Knight , Karl Battams

We surveyed 23 comets using the Infrared Array Camera on the Spitzer Space Telescope in wide filters centered at 3.6 and 4.5 microns. Emission in the 3.6 micron filter arises from sunlight scattered by dust grains; these images generally…

地球与行星天体物理 · 物理学 2015-06-16 William T. Reach , Michael S. Kelley , Jeremie Vaubaillon

Jupiter-family comet (JFC) P/2021 HS (PANSTARRS) only exhibits a coma within a few weeks of its perihelion passage at 0.8~au, which is atypical for a comet. Here we present an investigation into the underlying cause using serendipitous…

On 2007 October 29 the outbursting comet 17P/Holmes passed within 0.79 arcsec of a background star. We recorded the event using optical, narrowband photometry and detect a 3% to 4% dip in stellar brightness bracketing the time of closest…

地球与行星天体物理 · 物理学 2015-06-11 Pedro Lacerda , David Jewitt

We report results from broadband visible images of comet C/2012 S1 (ISON) obtained with the Hubble Space Telescope Wide Field Camera 3 on 2013 April 10. C/ISON's coma brightness follows a 1/{\rho} (where {\rho} is the projected distance…

We have analyzed Spitzer and NASA/IRTF 2 - 35 \mum spectra of the warm, ~350 K circumstellar dust around the nearby MS star {\eta} Corvi (F2V, 1.4 \pm 0.3 Gyr). The spectra show clear evidence for warm, water- and carbon-rich dust at ~3 AU…

太阳与恒星天体物理 · 物理学 2015-05-30 C. M. Lisse , M. C. Wyatt , C. H. Chen , A. Morlok , D. M. Watson , P. Manoj , P. Sheehan , T. M. Currie , P. Thebault , M. L. Sitko

We present observations of comet 67P/Churyumov-Gerasimenko during its 2021/22 apparition, aiming to investigate its dust and gas environment and compare the results with those obtained in 2015/16 using the same telescope. Quasi-simultaneous…

地球与行星天体物理 · 物理学 2025-09-17 V. Rosenbush , V. Kleshchonok , O. Ivanova , I. Luk'yanyk , C. Snodgrass , D. Gardener , L. Kolokolova , J. Markkanen , E. Shablovinskaya

We present an analysis of the photometric and spectroscopic data of the comet C/2012 S1 (ISON) observed at the heliocentric distances of 6.21\div 4.81 AU. The photometric observations were made with the 60-cm Zeiss-600 telescope (ICAMER,…

We present mid-infrared spectra and images from the GEMINI-N (+Michelle) observations of fragments SW3-[B] and SW3-[C] of the ecliptic (Jupiter Family) comet 73P/Schwassmann-Wachmann 3 pre-perihelion. We observed fragment B soon after an…

Thanks to the Rosetta mission, our understanding of comets has greatly improved. A very good opportunity to apply this knowledge appeared in early 2017 with the appearance of the Jupiter family comet 41P/TGK. We performed an observational…

地球与行星天体物理 · 物理学 2018-08-01 F. J. Pozuelos , E. Jehin , Y. Moulane , C. Opitom , J. Manfroid , Z. Benkhaldoun , M. Gillon

We have used the Spitzer Space Telescope Infrared Spectrograph (IRS) to observe the 5-37 micron thermal emission of comet 73P/Schwassmann-Wachmann 3 (SW3), components B and C. We obtained low spectral resolution (R ~ 100) data over the…