Abstract
Thermal observations of large asteroids at millimeter wavelengths have revealed high amplitude rotational lightcurves. Such lightcurves are important constraints on thermophysical models of asteroids, and provide unique insight into the nature of their surface and subsurface composition. A better understanding of asteroid surfaces provides insight into the composition, physical structures, and processing history of these surviving remnants from the formation of our solar system. In addition, detailed observations of the larger asteroids, accompanied by thermophysical models with appropriate temporal and spatial resolution, promise to decrease uncertainties in their flux predictions. Of particular interest are the near-Earth objects, which can be observed at large phase angles, permitting better assessment of the thermal response of their unilluminated surfaces. The high sensitivity of ALMA will enable us to detect many small bodies in all the major groups, to obtain lightcurves for a large sample of main-belt and near-Earth objects, to resolve the surfaces of some large objects, and to separate the emission from primary and secondary objects in binary pairs. In addition to the science goals of asteroid studies, these bodies may also prove useful operationally because those with known shapes and well-characterized lightcurves could be employed for flux calibration by ALMA and other high frequency instruments.
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References
Altenhoff, W.J., et al.: Millimeter-wavelength observations of minor planets. Astron. Astrophys. 287, 641–646 (1994)
Barerra-Pineda, P., et al.: Asteroid and minor bodies science with the Large Millimetric Telescope. Rev. Mex. Astron. Astrofís. (Ser. Conf.) 24, 188–191 (2005)
Belton, M.J.S., et al.: Bulk density of asteroid 243 Ida from the orbit of its satellite Dactyl. Nature 374, 785–788 (1996)
Belton, M.J.S., et al.: The discovery and orbit of 1993 (243)1 Dactyl. Icarus 120, 185–199 (1996)
Binzel, R.P., et al.: Geologic mapping of Vesta from 1994 Hubble Space Telescope images. Icarus 128, 95–103 (1997)
Burbine, T.H. et al.: Meteoritic parent bodies: their number and identification. In: Bottke, et al. (eds.) Asteroids III, pp. 653–667. University of Arizona Press (2002)
Bus, S.J., et al.: Visible-wavelength spectroscopy of asteroids. In: Bottke, et al. (eds.) Asteroids III, pp. 169–182. University of Arizona Press (2002)
Chamberlain, A.: NEO Discovery Statistics. http://neo.jpl.nasa.gov/stats. Cited 26 Jan 2007 (2007)
Chamberlain, A., et al.: Submillimeter lightcurves of Vesta. Icarus (2007, in press)
Chapman, C.R., et al.: Cratering on asteroids from Galileo and NEAR Shoemaker. In: Bottke, et al. (eds.) Asteroids III, pp. 315–330. University of Arizona Press (2002)
Chiang, E., et al.: A brief history of transneptunian space. In: Reipurth, et al. (eds.) Protostars and Planets V, pp. 895–911. University of Arizona Press (2007)
Drummond, J.D., et al.: Full adaptive optics images of asteroids Ceres and Vesta; Rotational poles and triaxial ellipsoid dimensions. Icarus 132, 80–99 (1998)
Ďurech, J., Kaasalainen, M.: Photometric signatures of highly nonconvex and binary asteroids. Astron. Astrophys. 404, 709–714 (2003)
Emery, J., et al.: Thermal emission spectroscopy (5.2–38 μm) of three Trojan asteroids with the Spitzer Space Telescope: Detection of fine-grained silicates. Icarus 182, 496–512 (2006)
Fernández, Y.R., et al.: The Albedo distribution of Jovian Trojan asteroids. Astron. J. 126, 1563–1574 (2003)
Johnston, K.J., et al.: The microwave spectra of the asteroids Pallas. Vesta, and Hygiea. Astron. J. 98, 335–340 (1989)
Kaasalainen, M., et al.: Models of twenty asteroids from photometric data. Icarus 159, 369–395 (2002)
Lacerda, P., Luu, J.: Analysis of the rotational properties of Kuiper Belt objects. Astron. J. 131, 2314–2326 (2006)
Li, J.-Y., et al.: Photometric analysis of 1 Ceres and surface mapping from HST observations. Icarus 182, 143–160 (2006)
Magri, C., et al.: A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999–2003. Icarus 186, 126–151 (2007)
Marchis, F.: A low density of 0.8 g cm−3 for the Trojan binary asteroid 617 Patroclus. Nature 439, 565–567 (2006)
Marjari, F., et al.: Origin and evolution of trojan asteroids. In: Bottke, et al. (eds.) Asteroids III, pp. 725–738. University of Arizona Press (2002)
Merline, W., et al.: Asteroids do have satellites. In: Bottke, et al. (eds.) Asteroids III, pp. 289–312. University of Arizona Press (2002)
Morbidelli, A., et al.: Chaotic capture of Jupiters Trojan asteroids in the early Solar System. Nature 435, 462–465 (2005)
Ostro, S.J., et al.: Asteroid Radar Astronomy. In: Bottke, et al. (eds.) Asteroids III, pp. 151–168. University of Arizona Press (2002)
Parker, J.W., et al.: Analysis of the first disk-resolved images of Ceres from ultraviolet observations with the Hubble Space Telescope. Astron. J. 123, 549–557 (2002)
Pravec, P., et al.: Asteroid Rotations, In: Bottke, et al. (eds.) Asteroids III, pp. 113–122. University of Arizona Press (2002)
Redman, R.O., et al.: Millimeter and submillimeter observations of the asteroid 4 Vesta. Astron. J. 104, 405–411 (1992)
Redman, R.O., et al.: High-quality photometry of asteroids at millimeter and submillimeter Wavelengths. Astron. J. 116, 1478–1490 (1998)
Richardson, D., Walsh, K.: Binary minor planets. Annu. Rev. Earth Planet. Sci. 34, 47–81 (2006)
Saito, J., et al.: Detailed images of asteroid 25143 Itokawa from Hayabusa. Science 312, 1341–1344 (2006)
Stokes, G.H., et al.: Near-Earth asteroid search programs. In: Bottke, et al. (eds.) Asteroids III, pp. 45–54. University of Arizona Press (2002)
Storrs, A.D., et al.: A closer look at main belt asteroids 1: WF/PC images. Icarus 173, 409–416 (2005)
Sullivan, R.J., et al.: Asteroid geology from Galileo and NEAR Shoemaker data. In: Bottke, et al. (eds.) Asteroids III, pp. 331–350. University of Arizona Press (2002)
Tedesco, E.F., et al.: The supplemental IRAS minor planet survey. Astron. J. 123, 1056–1085 (2002)
Thomas, P.C., et al.: Vesta: spin pole, size, and shape from HST images. Icarus 128, 88–94 (1997)
Veverka, J., et al.: Galileo’s encounter with 951 Gaspra: overview. Icarus 107, 2–17 (1994)
Zellner, B.H., et al.: Hubble Space Telescope images of asteroid 4 Vesta in 1994. Icarus 128, 83–87 (1997)
Zellner, N.E.B., et al.: Near-IR imaging of asteroid 4 Vesta. Icarus 177, 190–195 (2005)
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Lovell, A.J. (2008). Observations of asteroids with ALMA. In: Bachiller, R., Cernicharo, J. (eds) Science with the Atacama Large Millimeter Array. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-6935-2_35
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DOI: https://doi.org/10.1007/978-1-4020-6935-2_35
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