27 Euterpe

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27 Euterpe
27Euterpe (Lightcurve Inversion).png
Lightcurve-based 3D-model of Euterpe
Discovery [1]
Discovered by J. R. Hind
Discovery site George Bishop's Obs.
Discovery date8 November 1853
Designations
(27) Euterpe
Pronunciation /jˈtɜːrp/ [2]
Named after
Euterpe (Greek mythology) [3]
1945 KB
main-belt  ·(inner) [4]
Euterpe [5]
Adjectives Euterpean /jˈtɜːrpiən/ [6]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 163.48 yr (59,711 days)
Aphelion 2.7524 AU
Perihelion 1.9401 AU
2.3463 AU
Eccentricity 0.1731
3.59 yr (1,313 days)
170.66°
0° 16m 27.12s / day
Inclination 1.5837°
94.789°
356.55°
Physical characteristics
Dimensions124×75 km (occultation) [1]
96 km [1]
96.9 km [7]
105.80±7.23 km [8]
109.79±1.54 km [9]
118 km [10]
118.000±22.30 km [11]
Mass (1.67±1.01)×1018 kg [8]
Mean density
2.69±1.71 g/cm3 [8]
8.500 h [4]
10.377±0.008 h [12]
10.40193±0.00005 h [13]
10.404±0.001 h [4]
10.407±0.002 h [14]
10.4082±0.0001 h [15]
10.410±0.002 h [16] [17] [lower-alpha 1]
10.41 h [18]
0.20±0.03 [19]
0.2011±0.0582 [11]
0.215±0.033 [20]
0.234±0.008 [9]
0.298 [7]
Tholen = S [1]
SMASS = S [1]  · S [21] [4]
B–V = 0.878 [1]
U–B = 0.502 [1]
7.00 [1] [4] [7] [9] [11]  ·7.01±0.02 [15]
0.13" to 0.035"

    Euterpe, minor planet designation 27 Euterpe, is a stony asteroid and parent body of the Euterpe family, located in the inner asteroid belt, approximately 100 kilometers in diameter. It was discovered by English astronomer John Russell Hind at George Bishop's Observatory in London on 8 November 1853. The asteroid was named after Euterpe, the Muse of music in Greek mythology. [3] [22]

    Contents

    Euterpe is one of the brightest asteroids in the night sky. [23] It had an apparent magnitude of 8.5 during a perihelic opposition on 25 December 2015 when the asteroid was about 1 AU from Earth. [24] At the end of November 2022 it passed about 1.5 degrees from Uranus while in the constellation of Aries. [25] Based on the S-type spectra the composition appears stony. It has a cross-section size of around 100–120 km. 27 Euterpe is orbiting the Sun with a period of 3.59 years and is spinning on its axis once every 10.4 hours.

    It is the parent body of the Euterpe family ( 410 ), a stony inner-belt asteroid family of nearly 400 known members. [5] [26] :23Euterpe has been studied by radar. [27]

    Notes

    1. Lightcurve plot of 27 Euterpe, R. D. Stephens (lead) and B. D. Warner at the Palmer Divide Observatory (2000): rotation period 10.410±0.002 hours with a brightness amplitude of 0.21±0.01 mag. Summary figures at the LCDB

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    References

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