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187 Lamberta

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187 Lamberta
Discovery
Discovered byJ. Coggia, 1878
Discovery date11 April 1878
Designations
MPC designation(187) Lamberta
Pronunciation/læmˈbɜːrtə/
Alternative designationsA878 GB; 1946 LB;
1948 XR
Minor planet categoryMain belt
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc113.41 yr (41424 d)
Aphelion3.3856 AU (506.48 Gm)
Perihelion2.0695 AU (309.59 Gm)
Semi-major axis2.7276 AU (408.04 Gm)
Eccentricity0.24126
Orbital period (sidereal)4.50 yr (1645.3 d)
Mean anomaly217.42°
Mean motion0° 13 7.68 / day
Inclination10.588°
Longitude of ascending node21.707°
Argument of perihelion196.93°
Earth MOID1.07102 AU (160.222 Gm)
Jupiter MOID1.60105 AU (239.514 Gm)
TJupiter3.289
Physical characteristics
Mean diameter141±2 km
147.294±1.389 km
131.3±1.1 km
Flattening0.14
Mass(1.9±0.3)×10 kg
(1.80±0.85)×10 kg
Mean density1.28±0.22 g/cm
1.51±0.71 g/cm
Synodic rotation period10.67 h (0.445 d)
Geometric albedo0.052 (calculated)
0.044±0.007
0.0647 ± 0.0135
Spectral typeC (Tholen)
Absolute magnitude (H)8.40, 7.980

187 Lamberta is a main-belt asteroid that was discovered by Corsican-born French astronomer Jérôme Eugène Coggia on April 11, 1878, and named after the astronomer Johann Heinrich Lambert. It was the second of Coggia's five asteroid discoveries.

The spectrum matches a classification of a C-type asteroid, which may mean it has a composition of primitive carbonaceous materials. It is a dark object as indicated by the low albedo and has an estimated size of about 131 km.

Notes

  1. Flattening derived from the maximum aspect ratio (c/a): f = 1 c a {\displaystyle f=1-{\frac {c}{a}}} , where (c/a) = 0.86±0.07.

References

  1. ^ "187 Lamberta". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 12 May 2016.
  2. ^ P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. Astronomy & Astrophysics 54, A56
  3. ^ Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
  4. ^ Pravec, P.; et al. (May 2012), "Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations", Asteroids, Comets, Meteors 2012, Proceedings of the conference held May 16–20, 2012 in Niigata, Japan, no. 1667, Bibcode:2012LPICo1667.6089P. See Table 4.

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