4.4 Article

Spitzer Space Telescope Observations of the Nucleus of Comet 103P/Hartley 2

Journal

Publisher

IOP PUBLISHING LTD
DOI: 10.1086/605546

Keywords

-

Funding

  1. NASA
  2. Division Of Astronomical Sciences
  3. Direct For Mathematical & Physical Scien [908815] Funding Source: National Science Foundation

Ask authors/readers for more resources

We have used the Spitzer Space Telescope InfraRed Spectrograph (IRS) 22-mu m peakup array to observe thermal emission from the nucleus and trail of comet 103P/Hartley 2, the target of NASA's Deep Impact Extended Investigation (DIXI). The comet was observed on UT 2008 August 12 and 13, while 5.5 AU from the Sun. We obtained two 200 frame sets of photometric imaging over a 2.7 hr period. To within the errors of the measurement, we find no detection of any temporal variation between the two images. The comet showed extended emission beyond a point source in the form of a faint trail directed along the comet's antivelocity vector. After modeling and removing the trail emission, a NEATM model for the nuclear emission with beaming parameter of 0.95 +/- 0.20 indicates a small effective radius for the nucleus of 0.57 +/- 0.08 km and low geometric albedo 0.028 +/- 0.009 (1 sigma). With this nucleus size and a water production rate of 3 x 10(28) molecules s(-1) at perihelion, we estimate that similar to 100% of the surface area is actively emitting volatile material at perihelion. Reports of emission activity out to similar to 5 AU support our finding of a highly active nuclear surface. Compared to Deep Impact's first target, comet 9P/Tempel 1, Hartley 2's nucleus is one-fifth as wide (and about one-hundredth the mass) while producing a similar amount of outgassing at perihelion with about 13 times the active surface fraction. Unlike Tempel 1, comet Hartley 2 should be highly susceptible to jet driven spin-up torques, and so could be rotating at a much higher frequency. Since the amplitude of nongravitational forces are surprisingly similar for both comets, close to the ensemble average for ecliptic comets, we conclude that comet Hartley 2 must have a much more isotropic pattern of time-averaged outgassing from its nuclear surface. Barring a catastrophic breakup or major fragmentation event, the comet should be able to survive up to another 100 apparitions (similar to 700 yr) at its current rate of mass loss.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.4
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

Article Astronomy & Astrophysics

Extragalactic Magnetism with SOFIA (SALSA Legacy Program): The Magnetic Fields in the Multiphase Interstellar Medium of the Antennae Galaxies*

Enrique Lopez-Rodriguez, Alejandro S. Borlaff, Rainer Beck, William T. Reach, Sui Ann Mao, Evangelia Ntormousi, Konstantinos Tassis, Sergio Martin-Alvarez, Susan E. Clark, Daniel A. Dale, Ignacio del Moral-Castro

Summary: This study characterizes the morphology of the ordered magnetic fields in the interstellar medium (ISM) of the closest merging spiral galaxies, the Antennae galaxies. It reveals that the 154 μm magnetic fields are more ordered than the 11 cm magnetic fields. The turbulent-to-ordered 154 μm magnetic field increases at the galaxy cores and star-forming regions. It suggests that the amplified magnetic fields may support the gas flow between the galaxies and the tidal tail.

ASTROPHYSICAL JOURNAL LETTERS (2023)

Article Astronomy & Astrophysics

Analysis of Charon's spectrum at 2.21-μm from New Horizons/LEISA and Earth-based observations

Jason C. Cook, Silvia Protopapa, Cristina M. Dalle Ore, Dale P. Cruikshank, William M. Grundy, Carey M. Lisse, Bernard Schmitt, Anne Verbiscer, Kelsi N. Singer, John Spencer, S. Alan Stern, Harold A. Weaver

Summary: In this study, we examined the 2.21-mu m band of Charon using data obtained by New Horizons/LEISA. We found no significant variation in this band as Charon rotates. The 2.21-mu m band on Charon is several times weaker than on other moons, and we attribute it to NH4Cl based on the appearance of a weaker band at 2.24-mu m. Additionally, we observed two never-before-reported absorption features in Charon's spectrum at 1.60 and 1.63-mu m, which may also be explained by the presence of NH4Cl. If NH3-H2O ice mixtures are present on Charon, they must be a small fraction of the overall composition.

ICARUS (2023)

Article Astronomy & Astrophysics

A targeted search for Main Belt Comets

Lea Ferellec, Colin Snodgrass, Alan Fitzsimmons, Agata Rozek, Daniel Gardener, Richard Smith, Hissa Medeiros, Cyrielle Opitom, Henry H. Hsieh

Summary: Main Belt Comets (MBCs) show sublimation-driven activity while orbiting in the Main Asteroid Belt. MBCs and candidates exhibit a higher concentration of perihelion longitudes around 15 degrees compared to other objects in the Outer Main Belt (OMB). This characteristic may aid in the discovery of new candidates by observing objects in similar orbits.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2023)

Article Astronomy & Astrophysics

Wavelength-dependent Extinction and Grain Sizes in Dippers

Michael L. Sitko, Ray W. W. Russell, Zachary C. C. Long, Korash Assani, Monika Pikhartova, Ammar Bayyari, Carol A. A. Grady, Carey M. M. Lisse, Massimo Marengo, John P. P. Wisniewski, William C. C. Danchi

Summary: This study examines the internight variability of K2-discovered dippers using the SpeX spectrograph. The properties of the dust in these dippers differ from the diffuse interstellar medium and molecular clouds, but resemble those seen in the disks of young stellar objects.

ASTRONOMICAL JOURNAL (2023)

Article Astronomy & Astrophysics

Modeling CO Line Profiles in Shocks of W28 and IC 443

Nguyen Fuda, Le Ngoc Tram, William T. Reach

Summary: Molecular emission from SNR-molecular cloud interactions provides a tool for studying star formation and cosmic-ray production. CO emission, created by magnetohydrodynamic shock, is an effective tracer for slow-moving shocks into the inner clumps. In this study, a new theoretical framework is presented for predicting CO line profiles using the Paris-Durham 1D shock model.

ASTROPHYSICAL JOURNAL (2023)

Article Astronomy & Astrophysics

A Measurement of the Cosmic Optical Background and Diffuse Galactic Light Scaling from the R < 50 au New Horizons-LORRI Data

Teresa Symons, Michael Zemcov, Asantha Cooray, Carey Lisse, Andrew R. Poppe

Summary: Direct photometric measurements of the cosmic optical background (COB) provide a point of comparison for other measurement methodologies and models of cosmic structure formation, and allow for a cosmic consistency test to reveal additional sources of emission. However, measuring the COB from Earth has been challenging due to interference from scattered light in our solar system. In this study, data from the Long-Range Reconnaissance Imager on NASA's New Horizons mission was used to measure the COB, with the analysis accounting for various instrumental systematics and astrophysical foregrounds. The results suggest a higher light intensity than expected, calling for further measurements with more advanced instruments.

ASTROPHYSICAL JOURNAL (2023)

Article Astronomy & Astrophysics

Optical Spectropolarimetry of Binary Asteroid Didymos-Dimorphos before and after the DART Impact

Stefano Bagnulo, Zuri Gray, Mikael Granvik, Alberto Cellino, Ludmilla Kolokolova, Karri Muinonen, Olga Munoz, Cyrielle Opitom, Antti Penttila, Colin Snodgrass

Summary: We studied the Didymos-Dimorphos binary asteroid in spectropolarimetric mode to understand the characteristics of the ejected dust before and after the DART impact. Prior to impact, Didymos showed an increasing linear polarization with phase angle, reaching about 5% in the blue and 4.5% in the red. The polarization spectrum was anticorrelated with the reflectance spectrum, indicating it was an S-class asteroid. After impact, the level of polarization slightly decreased in both the blue and red bands, but continued to increase linearly with phase angle, similar to the measurements before impact. The lack of significant change in the polarization spectrum suggests that the wavelength dependence of polarization depends on the composition of the scattering material rather than its structure.

ASTROPHYSICAL JOURNAL LETTERS (2023)

Article Astronomy & Astrophysics

Tuning the Legacy Survey of Space and Time (LSST) Observing Strategy for Solar System Science

Megan E. Schwamb, R. Lynne Jones, Peter Yoachim, Kathryn Volk, Rosemary C. Dorsey, Cyrielle Opitom, Sarah Greenstreet, Tim Lister, Colin Snodgrass, Bryce T. Bolin, Laura Inno, Michele T. Bannister, Siegfried Eggl, Michael Solontoi, Michael S. P. Kelley, Mario Juric, Hsing Wen Lin, Darin Ragozzine, Pedro H. Bernardinelli, Steven R. Chesley, Tansu Daylan, Josef Durech, Wesley C. Fraser, Mikael Granvik, Matthew M. Knight, Carey M. Lisse, Renu Malhotra, William J. Oldroyd, Audrey Thirouin, Quanzhi Ye

Summary: The Vera C. Rubin Observatory is preparing for the Legacy Survey of Space and Time (LSST) in 2025, aiming to transform our understanding of the solar system by discovering and monitoring over five million small bodies. The LSST survey strategy plays a crucial role in the discovery and characterization of solar system minor planets and passing interstellar objects. To optimize the LSST survey strategy, a series of operation simulations have been conducted to explore different observing parameters and priorities. The impact of these simulated LSST observing strategies on studying the solar system's small body reservoirs has been examined, highlighting the importance of maximizing LSST solar system science.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2023)

Article Astronomy & Astrophysics

A retrospective analysis of mid-infrared observations of the Comet D/Shoemaker-Levy 9 and Wesley impacts on Jupiter

J. A. Sinclair, C. M. Lisse, G. S. Orton, M. Krishnamoorthy, L. N. Fletcher, J. Hora, C. Palotai, T. Hayward

Summary: We retrospectively analyzed Earth-based mid-infrared observations of Jupiter after its impacts by SL9 in July 1994 and the Wesley impactor in July 2009, using consistent data reduction and analysis methods. The SL9 impacts resulted in enhanced CH4 emissions at 7.9 μm and NH3 emissions at 8.5-11.5 μm, while the Wesley impact exhibited enhanced emissions at 8.8-11.5 μm and 18-19 μm. The different composition and altitude of the impacts indicate deeper penetration for SL9, with NH3 abundances about 40 times higher than in the Wesley impact. The absence of silicates in the Wesley impact suggests a different incident angle and entry angle for the impactor.

ICARUS (2023)

Article Astronomy & Astrophysics

Characterizing the nucleus of comet 162P/Siding Spring using ground-based photometry

A. Donaldson, R. Kokotanekova, A. Rozek, C. Snodgrass, D. Gardener, S. F. Green, N. Masoumzadeh, J. Robinson

Summary: This study reports new r-band nucleus light curves for comet 162P/Siding Spring, obtained in 2018, 2021, and 2022. A convex shape model of the nucleus is created by convex lightcurve inversion, suggesting a possible bilobed structure. A linear phase function and brightness interpolation for the nucleus are derived after correcting the light curves for rotational effects. Challenges associated with modelling comet nucleus shapes from light curves are highlighted, and the potential role of the Legacy Survey of Space and Time in alleviating these challenges is discussed.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2023)

Article Astronomy & Astrophysics

SOFIA plus FORCAST Lunar Legacy Project Processing Procedure

A. Arredondo, C. I. Honniball, P. G. Lucey, W. T. Reach, E. R. Malaret, A. Thorpe

Summary: The Lunar Legacy Project aims to detect and characterize the distribution of water on the Moon's surface using the 6 μm spectral band. Spectra were obtained from the Faint Object Infrared Camera for the SOFIA Telescope instrument between 2018 and 2022. This paper explains the necessary processing steps, including the use of the SOFIA Redux package and Python scripts written by the team, to reduce the raw data and create flux-calibrated spectra.

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC (2023)

Review Astronomy & Astrophysics

Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe

P. C. Brandt, E. Provornikova, S. D. Bale, A. Cocoros, R. DeMajistre, K. Dialynas, H. A. Elliott, S. Eriksson, B. Fields, A. Galli, M. E. Hill, M. Horanyi, T. Horbury, S. Hunziker, P. Kollmann, J. Kinnison, G. Fountain, S. M. Krimigis, W. S. Kurth, J. Linsky, C. M. Lisse, K. E. Mandt, W. Magnes, R. L. McNutt, J. Miller, E. Moebius, P. Mostafavi, M. Opher, L. Paxton, F. Plaschke, A. R. Poppe, E. C. Roelof, K. Runyon, S. Redfield, N. Schwadron, V. Sterken, P. Swaczyna, J. Szalay, D. Turner, H. Vannier, R. Wimmer-Schweingruber, P. Wurz, E. J. Zirnstein

Summary: This article provides a detailed overview of the knowledge gaps in our understanding of the interaction between the heliosphere and the largely unexplored Very Local Interstellar Medium (VLISM), as well as predictions of potential scientific discoveries in this field. The article discusses the new measurements needed to make progress in space physics, including in-situ plasma and pick-up ion measurements, direct sampling of VLISM properties, and remote imaging to discern the heliospheric shape and interaction with interstellar hydrogen. A 4-year NASA funded mission study reports the implementation of a pragmatic Interstellar Probe mission with a nominal design life of reaching 375 Astronomical Units (au), with likely operation out to 550 au.

SPACE SCIENCE REVIEWS (2023)

Article Astronomy & Astrophysics

The Distribution of Molecular Water in the Lunar South Polar Region Based upon 6 μm Spectroscopic Imaging

William T. Reach, Paul G. Lucey, Casey I. Honniball, Anicia Arredondo, Erick R. Malaret

Summary: The presence of water on the lunar surface is determined by the input and production of water through solar wind and meteoroid bombardment, as well as photodestruction and mobility across the surface. Using the Stratospheric Observatory for Infrared Astronomy (SOFIA), we observed variations in the distribution of water on the lunar nearside surface, with drier conditions at +28 degrees longitude and wetter conditions at -7 degrees longitude, decreasing towards the poles. Significant local enhancements were found in south-facing, high-altitude topographic features, including wet ridges, crater rims, and permanently shadowed polar regions.

PLANETARY SCIENCE JOURNAL (2023)

Article Engineering, Aerospace

Altamira Comet proof-of-concept

Greg Pass, Dan Goods, Pilar Fatas, Apoorv Khandelwal, Michael Skvarla, Noriaki Nakayamada, Karen Meech, Sonia Hernandez, Evan Hilgemann

Summary: This proof-of-concept presents a 21st century artwork that represents the evolution of human identity through the use of selfies. The artwork, called the Altamira Comet, aims to gather selfies from individuals around the world and create microscopic bust sculptures that will be launched into heliocentric orbit. The concept involves using advanced technological processes to fabricate each selfie sculpture the size of cosmic dust. Plans are also discussed to deploy the comet using a standard CubeSat deployer and eventually expand the participation to reach at least one billion global participants.

ACTA ASTRONAUTICA (2023)

Article Astronomy & Astrophysics

Physical modelling of near-Earth asteroid (23187) 2000 PN9 with ground-based optical and radar observations

L. Dover, S. C. Lowry, A. Rozek, B. Rozitis, S. L. Jackson, T. Zegmott, Yu N. Krugly, I. N. Belskaya, A. Fitzsimmons, S. F. Green, C. Snodgrass, P. R. Weissman, M. Brozovic, L. A. M. Benner, M. W. Busch, V. R. Ayvazian, V Chiorny, R. Ya Inasaridze, M. Krugov, S. Mykhailova, I Reva, J. Hibbert

Summary: This study presents a physical model and spin-state analysis of the potentially hazardous asteroid (23187) 2000 PN9. By collecting optical light curves and utilizing planetary radar data, a detailed shape model was developed to search for YORP acceleration. The results suggest that 2000 PN9 is a relatively large top-shaped body with a short sidereal rotation period. Although no evidence for rotational acceleration was found, the presence of small YORP torques cannot be ruled out. It is likely that 2000 PN9 is an object that has undergone YORP evolution.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2023)

No Data Available