Discovery [1] | |
---|---|
Discovered by | S. J. Bus |
Discovery site | Siding Spring Obs. |
Discovery date | 2 March 1981 |
Designations | |
(3000) Leonardo | |
Named after | Leonardo da Vinci [2] (Renaissance polymath) |
1981 EG19 ·1961 XB 1975 NK1 ·1979 UT4 1979 WC6 | |
main-belt [1] [3] ·(inner) background [4] | |
Orbital characteristics [3] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter 0 | |
Observation arc | 56.76 yr (20,731 d) |
Aphelion | 2.7755 AU |
Perihelion | 1.9268 AU |
2.3511 AU | |
Eccentricity | 0.1805 |
3.61 yr (1,317 d) | |
358.39° | |
0° 16m 24.24s / day | |
Inclination | 2.7514° |
200.98° | |
173.67° | |
Physical characteristics | |
Mean diameter | 9.044±1.725 km [5] 9.05±2.22 km [6] 9.777±0.277 km [7] 9.838±0.068 km [8] [9] 10.6±1.1 km [10] |
7.524±0.021 h [11] | |
0.05 [6] [12] 0.0585 [5] 0.06 [10] 0.115 [8] [9] 0.117 [7] | |
SMASS = B [3] [13] | |
13.60 [10] [12] 13.70 [1] [3] [13] [14] 13.80 [5] | |
3000 Leonardo, provisional designation 1981 EG19, is a carbonaceous background asteroid from the inner regions of the asteroid belt, approximately 9.5 kilometers (5.9 miles) in diameter. It was discovered on 2 March 1981, by American astronomer Schelte Bus at the Siding Spring Observatory in Australia. [1] The B-type asteroid has a rotation period of 7.5 hours. [13] It was named for the Italian polymath Leonardo da Vinci. [2]
Leonardo is a non-family asteroid from the main belt's background population. [4] It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.8 AU once every 3 years and 7 months (1,317 days; semi-major axis of 2.35 AU). Its orbit has an eccentricity of 0.18 and an inclination of 3° with respect to the ecliptic. [3] The body's observation arc begins with a precovery taken at the Goethe Link Observatory in December 1961, more than 19 years prior to its official discovery observation at Siding Spring. [1]
In 1986, 3000 Leonardo was observed to be at its predicted location. [15] It was one of 450 minor planets whose location was checked in a large observation campaign involving multiple sites and astronomers. [15] 3000 Leonard was visually observed by Roger E. Harvey on August 30, 1986 with a 73 cm Newtonian telescope from eastern North America (Concord, North Carolina in the United States). [15] [16]
This minor planet after the Italian polymath of the Renaissance Leonardo da Vinci (1452–1519) from Florence. He was a painter, sculptor, architect, musician, engineer and natural philosopher. The official naming citation was published by the Minor Planet Center on 29 September 1985 ( M.P.C. 10044). [17] He is also honored by both a lunar and a Martian crater ( Da Vinci and Da Vinci , respectively). [2] The asteroid is one of several early "kilo-numbered" minor planets that were dedicated to renowned scientists or institutions including: [18]
The sequence continues with the asteroids 5000 IAU (for the International Astronomical Union), 6000 United Nations (for the United Nations), 7000 Curie (for the pioneers on radioactivity, Marie and Pierre Curie), and 8000 Isaac Newton (for Isaac Newton), [18] while 9000 Hal (after HAL 9000 from 2001: A Space Odyssey) and 10000 Myriostos (after the Greek word for ten-thousandth, which is meant to honor all astronomers) were named based on their direct numeric accordance.
By 2001, 3000 Leonardo was one of 32 named minor planets named after painters and sculptors, and some other examples in this category include 3001 Michelangelo (the next named asteroid numerically), 4221 Picasso, and 4457 van Gogh. [19] Although these were classically named, the 1980s were a time of new concepts in naming, and it was a popular time to name minor planets after acronyms (such as 3568 ASCII) and one astronomer promoted more whimsical names including successfully naming one discovery after his pet. [19] However, there was a backlash against naming asteroids after pets, and the IAU does not recommend minor planets be named after pets. [20] [21]
At the time of 3000 Leonardo's discovery and naming only a few thousand asteroids had been discovered and named, it would not be until the 1990s and early 2000s when there was a massive spike in asteroid discoveries, with the peak year up to the year 2010, being 2000. [22] In the year 2000, over 40,000 minor planets were recorded, and in the years after many tens of thousands were discovered leading to almost 220,000 numbered minor planets by late 2009. [22]
Leonardo was one of 1341 main-belt asteroids observed between 1993 and 1999 as part of Small Main-Belt Asteroid Spectroscopic Survey (SMASSII). [23] In the SMASS taxonomy, it has a spectral type of a B-type asteroid, a "bright" carbonaceous body that is less common than the abundant C-type asteroids. [3]
In October 2015, a rotational lightcurve of Leonardo was obtained from photometric observations by astronomers at the University of Maryland using a 0.43-meter telescope at Mayhill, New Mexico ( H10 ). Lightcurve analysis gave a rotation period of 7.524±0.021 hours with a brightness variation of 0.26 magnitude ( U=2 ). [11] The result supersedes a tentative period determination by astronomers at Lindby Observatory ( K60 ) which gave a spin rate of 8.54 and an amplitude of 0.20 magnitude ( U=1 ). [13] [24]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Leonardo measures between 9.03 and 11 kilometers in diameter and its surface has an albedo between 0.05 and 0.117. [5] [6] [7] [8] [9] [10] [12] [14]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 (rather than for a carbonaceous one) and consequently calculates a shorter diameter of 5.41 kilometers based on an absolute magnitude of 13.7. [13]
4349 Tibúrcio, provisional designation 1989 LX, is a dark asteroid from the central region of the asteroid belt, approximately 29 kilometers in diameter. It was discovered on 5 June 1989, by German astronomer Werner Landgraf at ESO's La Silla Observatory in northern Chile.
1743 Schmidt, provisional designation 4109 P-L, is a dark background asteroid from the inner regions of the asteroid belt, approximately 19 kilometers in diameter. It was discovered during the Palomar–Leiden survey on 24 September 1960, by astronomers Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Tom Gehrels at Palomar Observatory in California. The C-type asteroid has a rotation period of 17.5 hours. It was named for the optician Bernhard Schmidt.
997 Priska, provisional designation 1923 NR, is a carbonaceous Adeonian asteroid from the central regions of the asteroid belt, approximately 19 kilometers in diameter. It was discovered on 12 July 1923, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid's name is a common German female name, unrelated to the discoverer's contemporaries.
2000 Herschel, provisional designation 1960 OA, is a stony Phocaea asteroid and a tumbling slow rotator from the inner regions of the asteroid belt, approximately 16 kilometers in diameter. It was discovered 29 July 1960, by German astronomer Joachim Schubart at Sonneberg Observatory in eastern Germany. The S-type asteroid has a long rotation period of 130 hours. It was named after astronomer William Herschel.
2007 McCuskey, provisional designation 1963 SQ, is a carbonaceous asteroid from the inner regions of the asteroid belt, approximately 22 kilometers in diameter. It was discovered on 22 September 1963, by astronomers of the Indiana Asteroid Program at Goethe Link Observatory near Brooklyn, Indiana, United States. The asteroid was later named after American astronomer Sidney McCuskey.
6433 Enya, provisional designation 1978 WC, is a stony background asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 18 November 1978, by Czech astronomer Antonín Mrkos at the Kleť Observatory in the Czech Republic. It was named for Irish musician Enya.
1159 Granada, provisional designation 1929 RD, is a dark background asteroid and relatively slow rotator from the inner regions of the asteroid belt, approximately 30 kilometers in diameter. It was discovered on 2 September 1929, by astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. The asteroid was named for the Spanish city and province of Granada.
11277 Ballard, provisional designation 1988 TW2, is a Phocaea asteroid from the inner regions of the asteroid belt, approximately 6.3 kilometers (3.9 miles) in diameter. It was discovered on 8 October 1988, by American astronomer couple Carolyn and Eugene Shoemaker at the Palomar Observatory in California. The assumed S-type asteroid has a rotation period of at least 10 hours. It was named for American marine scientist Robert Ballard.
1707 Chantal, provisional designation 1932 RL, is a stony background asteroid from the Florian region in the inner asteroid belt, approximately 7.5 kilometers in diameter. It was discovered on 8 September 1932, by astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle. The S-type asteroid has a rotation period of at least 10 hours. It was named for Chantal, the niece of Belgian astronomer Georges Roland.
1991 Darwin, provisional designation 1967 JL, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter.
1267 Geertruida, provisional designation 1930 HD, is a carbonaceous background asteroid from the inner regions of the asteroid belt, approximately 20 kilometers in diameter. Discovered by astronomer Hendrik van Gent at Johannesburg Observatory in 1930, the asteroid was later named after Geertruid Pels, sister of Dutch astronomer Gerrit Pels.
2571 Geisei, provisional designation 1981 UC, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered by Japanese astronomer Tsutomu Seki at Geisei Observatory on 23 October 1981, and named for the Japanese village of Geisei.
4000 Hipparchus is a dark background asteroid from the central regions of the asteroid belt, approximately 17 kilometers in diameter. It was discovered on 4 January 1989, by Japanese astronomers Seiji Ueda and Hiroshi Kaneda at the Kushiro Observatory on Hokkaido, Japan. The likely carbonaceous asteroid has a short rotation period of 3.4 hours. It was named for the ancient Greek astronomer Hipparchus.
1303 Luthera, provisional designation 1928 FP, is a dark asteroid and the parent body of the Luthera family, located in the outermost regions of the asteroid belt. It measures approximately 90 kilometers in diameter. The asteroid was discovered on 16 March 1928, by astronomer Friedrich Schwassmann at the Bergedorf Observatory in Hamburg, Germany, and later named after German astronomer Robert Luther.
1405 Sibelius, provisional designation 1936 RE, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 12 September 1936, by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland. The asteroid was named after composer Jean Sibelius.
1692 Subbotina, provisional designation 1936 QD, is a dark background asteroid from the central region of the asteroid belt, approximately 37 kilometers in diameter. The carbonaceous Cg-type asteroid has a rotation period of 9.2 hours. It was discovered by Grigory Neujmin at the Crimean Simeiz Observatory in 1936, and later named after Soviet mathematician and astronomer Mikhail Subbotin.
3823 Yorii, provisional designation 1988 EC1, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 11 kilometers in diameter.
4760 Jia-xiang, provisional designation 1981 GN1, is a background asteroid from the inner regions of the asteroid belt, approximately 5 kilometers (3 miles) in diameter. It was discovered on 1 April 1981, by astronomers at Harvard University's Oak Ridge Observatory in Massachusetts, United States. The presumed stony S-type asteroid was named after Chinese astronomer Zhang Jiaxiang. It has a rotation period of 14.96 hours.
7526 Ohtsuka, provisional designation 1993 AA, is a stony asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered by Japanese astronomer Takeshi Urata at Nihondaira Observatory Oohira Station, Japan, on 2 January 1993. The asteroid was named after Japanese astronomer Katsuhito Ohtsuka.
15224 Penttilä, provisional designation 1985 JG, is a dark background asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 15 May 1985, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Arizona, United States. The likely elongated asteroid has a rotation period of 4.4 hours. It was named after planetary scientist Antti Penttilä at the University of Helsinki.