Skip to main content Accessibility help
×
Hostname: page-component-8448b6f56d-mp689 Total loading time: 0 Render date: 2024-04-16T18:41:16.020Z Has data issue: false hasContentIssue false

1 - It's a small world

Published online by Cambridge University Press:  05 May 2015

Michael K. Shepard
Affiliation:
Bloomsburg University, Pennsylvania
Get access

Summary

Then I felt like some watcher of the skies

When a new planet swims into his ken;

John Keats, On first looking into Chapman's Homer

TRAIN STATION SIX

On the evening of October 6, 2008, Richard Kowalski was monitoring the search results of hundreds of images he and others routinely take each clear night with the 1.5 m Mt. Lemmon telescope. It is one of three telescopes used for the Catalina Sky Survey, an effort funded by NASA to discover new asteroids and comets. As on many other nights, a faint speck in the images, one of thousands, caught his attention – a new asteroid. After checking to see that it was not already known, it was dutifully given the cryptic provisional designation 8TA9D60 and reported to the Minor Planet Center in Cambridge, Massachusetts, the clearinghouse for all new asteroid and comet discoveries. Other observatories in Arizona and Australia were notified and quickly observed it. Dozens of new images were taken, giving enough information to calculate orbital elements and announce the discovery through a Minor Planet Electronic Circular. All of this happened within eight hours of the initial discovery and, by then, the object had a new name – 2008 TC3. Why the rush? Preliminary orbital calculations at the Minor Planet Center showed a 100% chance of impact in less than twelve hours.

In the eight hours between discovery and announcement, astronomer Steve Chesley at NASA's Jet Propulsion Laboratory (JPL) had been flagged and confirmed the initial assessment: the orbit of 2008 TC3 would intersect the Earth on 2008 Oct 07 02:46 UTC (Universal Time), less than twelve hours from the announcement, with an impact point over northern Sudan. In a stunning display of rapid international collaboration by professional and amateur astronomers around the world, hundreds of additional observations were made in the remaining hours and, one hour prior to impact, Paul Chodas – a colleague of Chesley's at JPL – reported a refined atmospheric entry time of 2008 Oct 07 02:44:28 UTC ± 15 seconds, with an impact time of 02:46:20 UTC ± 40 seconds.

Type
Chapter
Information
Asteroids
Relics of Ancient Time
, pp. 1 - 34
Publisher: Cambridge University Press
Print publication year: 2015

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

S., Chesley, P., Chodas, D., Yeomans. Asteroid 2008 TC3 strikes Earth: Predictions and observations agree. JPL News November 4, 2008. http://neo.jpl.nasa.gov/news/2008tc3.html
P., Jenniskens et al. The impact and recovery of asteroid 2008 TC3. Nature, 458 (2009) 485–488.Google Scholar
R., Kwok. The rock that fell to Earth. Nature, 458 (2009) 401–403. http://www.nature.com/news/2009/090325/full/458401a.html
Minor Planet Electronic Circular (MPEC 2008-T50) 2008 TC3. http://www.mmorplanetcenter.net/mpec/K08/K08T50.html
International Astronomical Union Circular (IAUC 6457). Elst-Pizarro cometary discovery connected to 1979 OW7. http://www.cbat.eps.harvard.edu/iauc/06400/06457.html
Minor Planet Electronic Circular (MCEC 1996-R07). Hawkins and McNaught discovery Elst-Pizarro. http://www.minorplanetcenter.net/mpec/J96/J96R07. html
P., Rincon. The girl who named a planet. Pluto: The discovery of Planet X (BBC News) January 13, 2006. http://news.bbc.co.uk/2/hi/science/nature/4596246.stm
International Astronomical Union definition of planet: http://www.iau.org/static/ archives/releases/pdf/iau0603.pdf
L5 Society: http://www.nss.org/resources/library/spacemovement/chapter05.htm
NEO groups: http://neo.jpl.nasa.gov/neo/groups.html
Number of Centaurs: http://ssd.jpl.nasa.gov/sbdb_query.cgi#x
Numbers of NEOs: http://neo.jpl.nasa.gov/stats/Voyager at Uranus, 1986, NASA JPL 400–268 7/85, http://er.jsc.nasa.gov/seh/ hersc.html
M., Brown. How I Killed Pluto and Why It Had It Coming (New York: Spiegel and Grau, 2012).Google Scholar
A promised transit of Vulcan. The Spectator, 52, March 15, 1879, p. 336.
A. M., Clerke. A Popular History of Astronomy During the Nineteenth Century, 4th edn (London: A.&C. Black, 1885).Google Scholar
V., Duckles. Sir William Herschel as a composer. Publ. Astron. Soc. Pacific, 74(436) (1962) 55–59.Google Scholar
G., Fodera-Serio, A., Manara, P., Sicoli. Giuseppe Piazzi and the discovery of Ceres. In Asteroids III, eds. W. F., Bottke Jr., A., Cellino, P., Paolicchi, R. P., Binzel (Tucson, AZ: University of Arizona Press, 2002), pp. 17–26.Google Scholar
J. L., Hilton. When did the asteroids become minor planets? http://aa.usno.navy. mil/faq/docs/minorplanets.php
H. S., Hogg.Out of old books: The Titius-Bode law and the discovery of Ceres. J. Roy. Soc. Canada, 42 (1948) 241–246.Google Scholar
M., Hoskin. Was William Herschel a deserter?J. History Astron., 35 (2004) 356–358.Google Scholar
H. S., Jones. The solar parallax and the mass of the Moon from observations of Eros at the opposition of 1931. Mem. Roy. Astron. Soc., 66 (1941) 11–66.Google Scholar
E. C., Pickering.Witt's Planet (433) Eros. Astron. Nachr., 148 (1899) 189–192.Google Scholar
W. H., Steavenson.Herschel's first 40-foot speculum. The Observatory, 50 (1927) 114–118.Google Scholar
C. W., Tombaugh.The search for the ninth planet, Pluto.Astron. Soc. Pacific Leaflets, 5 (1946) 73–80.Google Scholar
M., Conners, P., Wiegert, C., Veillet. Earth's Trojan asteroid. Nature, 475 (2011) 481–483.Google Scholar
H. H., Hsieh, D. C., Jewitt, Y. R., Fernandez.The strange case of 133P/Elst-Pizarro: A comet among the asteroids.Astron. J., 127 (2004) 2997–3017.Google Scholar
D., Jewitt, J., Luu. Discovery of the candidate Kuiper Belt object 1992 QB1. Nature, 362 (1993) 730–732.Google Scholar
C., Kowal. A Solar System survey. Icarus, 77 (1989) 118–123.Google Scholar
J., Luu et al. A new dynamical class of object in the outer Solar System. Nature, 387 (1997) 573–575.Google Scholar
E. M., Shoemaker, C. S., Shoemaker, R. F., Wolfe.Trojan Asteroids: Populations, dynamical structure, and origin of the L4 and L5 swarms. In Asteroids II, eds. R. P., Binzel, T., Gehrels, M. S., Matthews (Tucson, AZ: University of Arizona Press, 1989), pp. 487–523.Google Scholar
/A. J., Steffi, N. J., Cunningham, A. B., Shinn, S. A., Stern.A search for Vulcanoids with the STEREO Heliospheric Imager.Icarus, 233 (2013) 48–56.Google Scholar
D. J., Tholen, R. J., Whiteley.Results from NEO searches at small solar elongations.Bull. Amer. Astron. Soc., 30 (1998) 1041.Google Scholar
F., Yoshida, T., Nakamura. Size distribution of faint Jovian L4 Trojan asteroids.
Astron., J., 130 (2005) 2900–2911.
Sagan quote: C., Sagan. Cosmos (New York: Random House, 1980), p. 64.Google Scholar
Kepler quote: J., Kepler. Mysterium Cosmographicum (The Secret of the Universe) (Tübingen, 1596), pp. 7–8; translated by A. M., Duncan (New York: Abaris Books, 1981), pp. 63–64.Google Scholar
Gregory quote: D., Gregory. The Elements of Astronomy (London, 1715), p. 2. https://archive.org/details/elementsofastron00greg
On the symbol for Irene: J. R., Hind.On the discovery of a fourth new planet, at Mr. Bishop's observatory, Regent's Park.Mon. Not. Roy. Astron. Soc., 11 (1851) 171.Google Scholar
Piazzi quote on his discovery: G., Fodera-Serio et al. Giuseppe Piazzi and the discovery of Ceres. In Asteroids III, eds. W. F., Bottke Jr., A., Cellino, P., Paolicchi, R. P., Binzel (Tucson, AZ: University of Arizona Press, 2002), pp. 17–26 (quoted p. 19).Google Scholar
Fodera-Serio quote: Ibid. p. 22.

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×