The 2014 ALMA Long Baseline Campaign: Observations of Asteroid 3 Juno at 60 Kilometer Resolution
Date Issued
2015
Author(s)
ALMA Partnership
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Hunter, T. R.
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Kneissl, R.
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Moullet, A.
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Brogan, C. L.
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Fomalont, E. B.
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Vlahakis, C.
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Asaki, Y.
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Barkats, D.
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Dent, W. R. F.
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Hills, R. E.
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Hirota, A.
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Hodge, J. A.
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Impellizzeri, C. M. V.
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Lucas, R.
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Marcelino, N.
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Matsushita, S.
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Nakanishi, K.
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Pérez, L. M.
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Phillips, N.
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Richards, A. M. S.
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Toledo, I.
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Aladro, R.
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Broguiere, D.
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Cortes, J. R.
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Cortes, P. C.
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Espada, D.
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Galarza, F.
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Garcia-Appadoo, D.
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Guzman-Ramirez, L.
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Hales, A. S.
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Humphreys, E. M.
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Jung, T.
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Kameno, S.
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Laing, R. A.
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Leon, S.
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Marconi, G.
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Mignano, A.
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Nikolic, B.
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Nyman, L. -A.
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Radiszcz, M.
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Remijan, A.
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Rodón, J. A.
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Sawada, T.
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Takahashi, S.
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Tilanus, R. P. J.
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Vila Vilaro, B.
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Watson, L. C.
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Wiklind, T.
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De Gregorio-Monsalvo, I.
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Di Francesco, J.
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Mangum, J.
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Francke, H.
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Gallardo, J.
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Garcia, J.
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Gonzalez, S.
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Hill, T.
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Kaminski, T.
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Kurono, Y.
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Lopez, C.
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Morales, F.
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Plarre, K.
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Randall, S.
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van kempen, T.
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Videla, L.
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Villard, E.
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Andreani, P.
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Hibbard, J. E.
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Tatematsu, K.
Description
This paper makes use of the following ALMA data set: ADS/JAO.ALMA#2011.0.00013.SV. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This research has made use of NASA's Astrophysics Data System. We thank Thomas Müller, Mark Gurwell, Bryan Butler, Rafael Hiriart, Ralph Marson, Dirk Petry, and Vivek Dhawan for useful discussions. Facilities: ALMA.
Abstract
We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm continuum images of the asteroid 3 Juno obtained with an angular resolution of 0\buildrel{\prime\prime}\over{.} 042 (60 km at 1.97 AU). The data were obtained over a single 4.4 hr interval, which covers 60% of the 7.2 hr rotation period, approximately centered on local transit. A sequence of 10 consecutive images reveals continuous changes in the asteroid's profile and apparent shape, in good agreement with the sky projection of the three-dimensional model of the Database of Asteroid Models from Inversion Techniques. We measure a geometric mean diameter of 259 ± 4 km, in good agreement with past estimates from a variety of techniques and wavelengths. Due to the viewing angle and inclination of the rotational pole, the southern hemisphere dominates all of the images. The median peak brightness temperature is 215 ± 13 K, while the median over the whole surface is 197 ± 15 K. With the unprecedented resolution of ALMA, we find that the brightness temperature varies across the surface with higher values correlated to the subsolar point and afternoon areas and lower values beyond the evening terminator. The dominance of the subsolar point is accentuated in the final four images, suggesting a reduction in the thermal inertia of the regolith at the corresponding longitudes, which are possibly correlated to the location of the putative large impact crater. These results demonstrate ALMA's potential to resolve thermal emission from the surface of main belt asteroids and to measure accurately their position, geometric shape, rotational period, and soil characteristics.
Volume
808
Issue
1
Start page
L2
Issn Identifier
2041-8205
Ads BibCode
2015ApJ...808L...2A
Rights
open.access
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