Discovery [1] [2] | |
---|---|
Discovered by | M. F. Wolf A. Schwassmann |
Discovery site | Heidelberg Obs. |
Discovery date | 31 October 1899 |
Designations | |
(449) Hamburga | |
Pronunciation | /hæmˈbɜːrɡə/ |
Named after | Hamburg [3] (German city) |
1899 EU ·1947 OA 1948 TO ·A901 EA | |
main-belt ·(middle) [4] background [5] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 117.91 yr (43,066 days) |
Aphelion | 2.9931 AU |
Perihelion | 2.1097 AU |
2.5514 AU | |
Eccentricity | 0.1731 |
4.08 yr (1,489 days) | |
228.86° | |
0° 14m 30.48s / day | |
Inclination | 3.0847° |
85.923° | |
47.281° | |
Physical characteristics | |
Dimensions | 55.09±14.25 km [6] 63.61±0.75 km [7] 66.76 ± 4.82 km [8] 77.90±22.29 km [9] 80.83±17.91 km [10] 85.59±1.9 km [11] |
Mass | (1.57±1.40)×1018 kg [8] |
18.145±0.005 h [12] 18.263±0.004 h [13] | |
0.03±0.02 [9] 0.033±0.009 [10] 0.0393±0.002 [11] 0.07±0.02 [6] 0.072±0.002 [7] | |
Tholen = C [1] [4] · C [14] B–V = 0.701 [1] U–B = 0.378 [1] | |
9.43±0.01 [4] [15] [16] ·9.47 [1] [7] [9] [11] ·9.79 [6] ·9.79±0.07 [17] ·9.80 [10] | |
Hamburga (minor planet designation: 449 Hamburga) is a carbonaceous asteroid from the background population of the intermediate asteroid belt, approximately 75 kilometers in diameter. It was discovered by German astronomers Max Wolf and Friedrich Schwassmann at Heidelberg Observatory on 31 October 1899, and later named after the city of Hamburg in Germany. [3] [2]
449 was a proposed target for the 1980s-1990s space probe mission proposal CRAF.
Hamburga is classified as a C-type asteroid and is probably composed of carbonaceous material. It is named for the city of Hamburg in Germany. [3] The name was announced in 1901 during a festival held by the Mathematical Society of Hamburg. [3]
449 Hamburga was identified as one of three asteroids that were likely to be a parent body for chondrites along with 304 Olga and 335 Roberta. [18] All three asteroids were known to have low-albedo (not reflect as much light) and be close to "meteorite producing resonances". [18] Chrondrites are the most common type of meteor found on Earth, accounting for over 80% of all meteors. [19] They are named for the tiny spherical silicate particles that are found inside them (those particles are called chondrules). [19]
In the 1980s and 1990s, NASA considered a spacecraft mission to the asteroid. [20] The mission plan called for a launch in 1995 and a flyby of Hamburga in early 1998. The McDonald's chain of restaurants expressed an interest in sponsoring the mission, due to the accidental similarity of the asteroid's name to the food item "hamburger", which was discussed in exploratory meetings between themselves and NASA. [21] [22]
In August 1988 in the United States' city of Baltimore, P. Weissman addressed the International Astronomical Union on a mission to this asteroid (449), a mission which also include a rendezvous with Comet Kopf. [23] See Comet Rendezvous Asteroid Flyby for more on the mission to the comet. This mission can also be compared to Rosetta, which successfully flew by two minor planets and orbited a Comet during its approach to the Sun in the early 21st century. P. Weissman later worked on the Rosetta mission. [24]
It was predicted that 449 occulted the star HIP 1424 in July 2013. [25] Stellar occultations can allow a chord to be calculated.
An asteroid occultation was predicted for 18 Oct 2018 with the magnitude 12 star UCAC4-557-042266. [26]
449 Hamburga has been observed to occult 15 stars between 1998 and 2023.
Maja is a carbonaceous background asteroid from the central regions of the asteroid belt, approximately 71 kilometers in diameter. It was discovered on 9 April 1861, by American astronomer Horace Tuttle at the Harvard College Observatory in Cambridge, Massachusetts, United States. The asteroid was named after Maia from Greek mythology.
Xanthippe is a dark background asteroid from the central regions of the asteroid belt, approximately 120 kilometers in diameter. It was discovered on 22 November 1875, by Austrian astronomer Johann Palisa at the Austrian Naval Observatory, in what is now Croatia. It is named after Xanthippe, the wife of the Greek philosopher Socrates.
Rhodope is a dark background asteroid from the central region of the asteroid belt, approximately 55 kilometers in diameter. It was discovered on 15 August 1876, by German–American astronomer Christian Peters at the Litchfield Observatory in Clinton, New York, United States. The asteroid was named after Queen Rhodope from Greek mythology.
Edith, provisional designation 1903 MH, is a carbonaceous background asteroid from the outer regions of the asteroid belt, approximately 83 kilometers in diameter. It was discovered on 22 September 1903, by American astronomer Raymond Dugan at the Heidelberg-Königstuhl State Observatory in southwest Germany, who named it after his sister Edith Eveleth.
La Paz, provisional designation 1923 PD, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 40 kilometers in diameter. It was discovered on 31 October 1923, by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory and named after the city La Paz in Bolivia.
1015 Christa, provisional designation 1924 QF, is a dark background asteroid from the outermost regions of the asteroid belt, approximately 96 kilometers in diameter. It was discovered on 31 January 1924, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The meaning of this asteroids's name is unknown.
1057 Wanda, provisional designation 1925 QB, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 43 kilometers in diameter. It was discovered by Grigory Shajn at the Simeiz Observatory in 1925, and later named after Polish–Soviet writer Wanda Wasilewska. The asteroid has a rotation period of 28.8 hours.
1128 Astrid, provisional designation 1929 EB, is a carbonaceous Astridian asteroid from the central region of the asteroid belt. It is the parent body of the Astrid family and measures approximately 40 kilometers in diameter.
1295 Deflotte, provisional designation 1933 WD, is a carbonaceous asteroid from the outer regions of the asteroid belt, approximately 48 kilometers in diameter. It was discovered on 25 November 1933, by French astronomer Louis Boyer at the Algiers Observatory in Algeria, North Africa. The asteroid was named after the discoverer's nephew.
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.
7225 Huntress, provisional designation 1983 BH, is a binary Florian asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered on 22 January 1983, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Flagstaff, Arizona, United States. It is named after astrochemist Wesley Huntress.
1309 Hyperborea is a carbonaceous background asteroid from the outermost regions of the asteroid belt, approximately 57 kilometers in diameter. It was discovered on 11 October 1931, by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula, and given the provisional designation 1931 TO. The asteroid was named after Hyperborea, the northern homeland of a Greek mythical race of giants.
1200 Imperatrix is a carbonaceous Hygiean asteroid from the outer regions of the asteroid belt, approximately 40 kilometres (25 mi) in diameter. It was discovered by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory on 14 September 1931. The asteroid was named after the Latin word for empress.
1347 Patria, provisional designation 1931 VW, is a carbonaceous asteroid from the background population of the central asteroid belt, approximately 32 kilometers in diameter. It was discovered on 6 November 1931, by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula. The asteroid was named for the Latin word of fatherland.
1197 Rhodesia, provisional designation 1931 LD, is a dark background asteroid from the outer regions of the asteroid belt, approximately 48 kilometers in diameter. It was discovered on 9 June 1931, by South African astronomer Cyril Jackson at the Union Observatory in Johannesburg. The likely C-type asteroid has a rotation period of 16.1 hours. It was named for Rhodesia, a former British colony and unrecognised state, which is now Zimbabwe.
1262 Sniadeckia, provisional designation 1933 FE, is a carbonaceous background asteroid from the asteroid belt's outer regions, approximately 54 kilometers in diameter. It was discovered on 23 March 1933, by Belgian astronomer Sylvain Arend at the Royal Observatory of Belgium in Uccle. The asteroid was named for Polish astronomer Jan Śniadecki. It has a notably low eccentricity of only 0.005.
1330 Spiridonia, provisional designation 1925 DB, is a dark background asteroid of primitive composition, located in the outer regions of the asteroid belt, approximately 65 kilometers in diameter. It was discovered on 17 February 1925, by Soviet astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula. The asteroid was named after the discoverer's brother-in-law, Spiridon Zaslavskij.
5176 Yoichi, provisional designation 1989 AU, is a 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 elongated asteroid has a brightness variation of 0.45 magnitude, and occulted a star in the constellation Cetus in November 2014. It was named for the Japanese town of Yoichi.
3823 Yorii, provisional designation 1988 EC1, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 11 kilometers in diameter.
861 Aïda is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 65 kilometers in diameter. It was discovered on 22 January 1917, by German astronomer Max Wolf at Heidelberg Observatory in southwest Germany, and given the provisional designation 1917 BE. It was named after the Italian opera Aida.