1070 Tunica

Dark background asteroid From Wikipedia, the free encyclopedia

1070 Tunica, provisional designation 1926 RB, is a dark background asteroid from the outer regions of the asteroid belt, approximately 35 kilometers in diameter. It was discovered on 1 September 1926, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany.[15] The asteroid was named after Petrorhagia, a flowering plant also known as "Tunica".[3]

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1070 Tunica
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date1 September 1926
Designations
(1070) Tunica
Pronunciation/ˈtjuːnɪkə/[2]
Named after
Petrorhagia[3]
(flowering plant)
1926 RB Â· A903 SA
main-belt Â· (outer)[1][4]
background[5] Â· Ursula[6]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc114.03 yr (41,649 days)
Aphelion3.4882 AU
Perihelion2.9764 AU
3.2323 AU
Eccentricity0.0792
5.81 yr (2,123 days)
259.51°
0° 10m 10.56s / day
Inclination16.963°
165.32°
189.81°
Physical characteristics
Dimensions33.77±8.89 km[7]
33.79 km (calculated)[4]
36.68±0.86 km[8]
39.10±0.64 km[9]
39.131±0.423 km[10]
44.135±1.028 km[11]
15.673±0.0067 h[12]
15.8±1.0 h[13]
0.0476±0.0014[11]
0.057 (assumed)[4]
0.061±0.003[10]
0.068±0.003[9]
0.07±0.04[7]
0.076±0.011[8]
C (assumed)[4]
10.60[8][9] Â· 10.634±0.001 (R)[12] Â· 10.70[7][11] Â· 10.76±0.29[14] Â· 10.8[1] Â· 11.08[4]
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Orbit and classification

Tunica is a non-family asteroid from the main belt's background population.[5] Conversely, it has also been considered a core member of the Ursula family.[6] It orbits the Sun in the outer main-belt at a distance of 3.0–3.5 AU once every 5 years and 10 months (2,123 days; semi-major axis of 3.23 AU). Its orbit has an eccentricity of 0.08 and an inclination of 17° with respect to the ecliptic.[1]

The body's observation arc begins with its identification as A903 SA at Heidelberg in September 1903, or 23 years prior to its official discovery observation.[15]

Physical characteristics

Tunica is an assumed C-type asteroid.[4]

Rotation period

In May 2017, a rotational lightcurve of Tunica was obtained from photometric observations by French amateur astronomer René Roy. Lightcurve analysis gave a rotation period of 15.8 hours with a brightness variation of 0.24 magnitude (U=2-).[13] Another lightcurve obtained in the R-band by astronomers at the Palomar Transient Factory in February 2010 gave a period of 15.673 hours and an amplitude of 0.32 magnitude (U=2).[12]

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Tunica measures between 33.77 and 44.135 kilometers in diameter and its surface has an albedo between 0.0476 and 0.076.[7][8][9][10][11]

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 33.79 kilometers based on an absolute magnitude of 11.08.[4]

Naming

This minor planet was named after "Tunica" (Petrorhagia), a flowering plant derived from the common gillyflower.[3]

Reinmuth's flowers

Due to his many discoveries, Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between (1009) and (1200). This list also contained a sequence of 28 asteroids, starting with 1054 Forsytia, that were all named after plants, in particular flowering plants (also see list of minor planets named after animals and plants).[16]

References

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