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8 - Terra incognita

Published online by Cambridge University Press:  05 May 2015

Michael K. Shepard
Affiliation:
Bloomsburg University, Pennsylvania
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Summary

Here be dragons.

Unknown

ARECIBO RADAR OBSERVATORY

Hidden deep in the northwestern rain forests of Puerto Rico, near the coastal city of Arecibo, is one of the technological wonders of man – the Arecibo Observatory, part of the National Astronomy and Ionosphere Center, or NAIC for short. The observatory is roughly an hour and a half drive west of San Juan at the terminus of highway PR-625. The last few miles of the trip wind precariously through small neighborhoods on narrow roads. The roads follow the hill and hollow karst terrain as a roller coaster might – up and down, left and right – and the effect on those inclined to motion sickness is just as wretched.

Because the topography is so rugged, you don't see any part of the enormous antenna until you pull up to the gate. Even then, the full effect isn't felt until you walk the hill to the Visitor Center, or are invited to visit the control room on the edge of the dish. Once there, though, the sight of it is powerful. Like a cybernetic prosthesis, the antenna dish appears to fit organically within the terrain.

The dish itself is not a solid object. Instead, hundreds of steel cables, parallel but separated from each other by a meter or so, are strung across a natural hollow and allowed to hang, creating a concave web. Nearly 40,000 lightweight aluminum screens, each about one by two meters, are set on top of the cables to create a giant, floating mesh. Each screen is precisely aligned by hand so that the entire structure deviates from a true spherical shape by less than a few millimeters anywhere.

The gauze-like metallic mesh has a couple of advantages over solid antennas. The telescope is designed to detect microwaves with wavelengths of tens of centimeters. Waves that large cannot pass through a fine screen mesh – it might as well be solid.

Type
Chapter
Information
Asteroids
Relics of Ancient Time
, pp. 219 - 252
Publisher: Cambridge University Press
Print publication year: 2015

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References

Arecibo Observatory: http://www.naic.edu
Goldstone Solar System Radar Group: http://gssr.jpl.nasa.gov/
DAMIT website asteroid shape models: http://astro.troja.mff.cuni.cz/projects/asteroids3D/web.php
Discovery of 90 Antiope moon: International Astronomical Union Circular (IAUC) 7503
Discovery of moon around 2000 DP107: IAUC 7504
Lutetia flyby compared to ground-based data press release: http://www.boulder.swri.edu/merline/press/lutetia-press-release-merline-100610-v1-text.pdf
Minor Planet Center lightcurve database: http://www.minorplanetcenter.net/iau/lists/LightcurveDat.html
B. A., Campbell. Radar Remote Sensing of Planetary Surfaces (Cambridge, UK: Cambridge University Press, 2002).Google Scholar
R., Nugent (ed.). Chasing the Shadow: The IOTA Occultation Observer's Manual. The Complete Guide to Observing Lunar, Grazing, and Asteroid Occultations (International Occultation Timing Association, 2007).
B. D., Warner. A Practical Guide to Lightcurve Photometry and Analysis (New York: Springer, 2006).Google Scholar
H. N., Russell. On the light-variations of asteroids and satellites. Astrophys. J., 24 (1906) 1–18.Google Scholar
S. D., Sinvhal, N. B., Sanwal, M. C., Pande. Observations of the occultation of BD -5° 5863 by Pallas. The Observatory, 92 (1962) 16–17.Google Scholar
G. E., Taylor. Diameters of minor planets. The Observatory, 92 (1962) 17–20.Google Scholar
J. M., Beckers. Adaptive optics for astronomy: Principles, performance, and applications. Annu. Rev. Astron. Astrophys., 31 (1993) 13–62.Google Scholar
M. J. S., Belton et al. Galileo's encounter with 243 Ida: An overview of the imaging experiment. Icarus, 120 (1996) 1–19.Google Scholar
B., Carry et al. The KOALA shape modeling technique validated at 21 Lutetia by ESA Rosetta mission. Division of Planetary Sciences Meeting (2010).
H., Demura et al. Pole and global shape of 25143 Itokawa. Science, 312 (2006) 1347–1349.Google Scholar
J., Durech, V., Sidorin, M., Kaasalainen. DAMIT: A database of asteroid models. Astron. Astrophys., 513 (2010) 1–13.Google Scholar
A., Fujiwara et al. The rubble-pile asteroid Itokawa as observed by Hayabusa. Science, 312 (2006) 1330–1334.Google Scholar
S., Hudson. Three-dimensional reconstruction of asteroids from radar observations. Remote Sens. Rev., 8 (1994) 195–203.Google Scholar
R. S., Hudson, S. J., Ostro. Shape of asteroid 4769 Castalia (1989 PB) from inversion of radar images. Science, 263 (1994) 940–943.Google Scholar
M., Kaasalainen, J., Torppa. Optimization methods for asteroid lightcurve inversion 1. Shape determination. Icarus, 153 (2001) 24–36.Google Scholar
M., Kaasalainen, J., Torppa, K., Muinonen. Optimization methods for asteroid lightcurve inversion 2. The complete inverse problem. Icarus, 153 (2001) 37–51.Google Scholar
L., Lewin. Letter symbols to designate microwave bands. IEEE Trans. Microwave Theory Tech., 12 (1964) 551.Google Scholar
S. C., Lowry et al. Direct detection of the asteroidal YORP Effect. Science, 316 (2007) 272–274.Google Scholar
F., Marchis, P., Descamps, D., Hestroffer, J., Berthier. Discovery of the triple asteroidal system 87 Sylvia. Nature, 436 (2005) 822–824.Google Scholar
W. J., Merline et al. Discovery of a moon orbiting the asteroid 45 Eugenia. Nature, 401(1999)565–568.Google Scholar
M., Nolan et al. Arecibo radar imaging of 2001 SN263: A near-Earth triple asteroid system. Asteroids, Comets, Meteors Meeting (2008), abstract #8258.
S. J., Ostro et al. Asteroid radar astronomy. In Asteroids III, eds. W. F., Bottke Jr., A., Cellino, P., Paolicchi, R. P., Binzel (Tucson, AZ: University of Arizona Press, 2002), pp. 151–168.Google Scholar
S. J., Ostro et al. Radar images of asteroid 1989 PB. Science, 248 (1990) 1523–1528.Google Scholar
S. J., Ostro et al. DP107. IAU Circular, 7496(2) (2000). See also IAUC 7503.Google Scholar
S. J., Ostro et al. Radar observations of asteroid 25143 Itokawa (1998 SF36). Meteor. Planet Sci, 39 (2004) 407–424.Google Scholar
S. J., Ostro et al. Radar observations of Itokawa in 2004 and improved shape estimation. Meteor. Planet. Sci., 40 (2005) 1563–1574.Google Scholar
P., Pravec et al. Two-period lightcurves of 1996 FG3, 1998 PG, and (5407) 1992 AX: One probable and two possible binary asteroids. Icarus, 146 (2000) 190–203.Google Scholar
D. P., Rubincam. Radiative spin-up and spin-down of small asteroids. Icarus, 148 (2000) 2–11.Google Scholar
M. K., Shepard et al. Multi-wavelength observations of asteroid Ra-Shalom. Icarus, 193 (2008) 20–38.Google Scholar
P. A., Taylor et al. Spin rate of asteroid (54509) 2000 PH5 increasing due to the YORP Effect. Science, 316 (2007) 274–277.Google Scholar
J., Veverka, M., Belton, K., Klaasen, C., Chapman. Galileo's encounter with 951 Gaspra: Overview. Icarus, 107 (1994) 2–17.Google Scholar
Russell quote. H. N., Russell. On the light-variations of asteroids and satellites. Astrophys. J., 24 (1906) p. 18.Google Scholar

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