277 Elvira

277 Elvira
	A three-dimensional model of 277 Elvira based on its light curve
Discovery
Discovered by	Auguste Charlois
Discovery date	3 May 1888
Designations
MPC designation	(277) Elvira
Alternative designations	A888 JA
Minor planet category	Main belt (Koronis)
Orbital characteristics
	Epoch 31 July 2016 (JD 2457600.5)
	Uncertainty parameter 0
Observation arc	116.65 yr (42607 d)
\|{{{apsis}}}\|helion}}	3.14812 astronomical unit\|AU (470.952 Gm)
\|{{{apsis}}}\|helion}}	2.62032 AU (391.994 Gm)
Semi-major axis	2.88422 AU (431.473 Gm)
Eccentricity	0.091498
Orbital period	4.90 yr (1789.1 d)
Mean anomaly	266.399°
Mean motion	0° 12m 4.378s / day
Inclination	1.16250°
Longitude of ascending node	231.271°
\|{{{apsis}}}\|helion}}	137.520°
Physical characteristics
Dimensions	27.19±0.9 km; 27.19 km
Rotation period	29.69 h (1.237 d)
Geometric albedo	0.2770±0.020; 0.277
Absolute magnitude (H)	9.84

Short description: Main-belt asteroid

Elvira (minor planet designation: 277 Elvira) is a typical main belt asteroid and is a member of the Koronis asteroid family. It was discovered by Auguste Charlois on 3 May 1888 in Nice. (277) Elvira is possibly named for a character in Alphonse de Lamartine's Méditations poétiques (1820) and Harmonies poétiques et religieuses (1830).^[3]

A group of astronomers, including Lucy D’Escoffier Crespo da Silva and Richard P. Binzel, used observations made between 1998 through 2000 to determine the spin-vector alignment of the Koronis family of asteroids, including 277 Elvira. The collaborative work resulted in the creation of 61 new individual rotation lightcurves to augment previous published observations.^[4]

Measurements of the thermal inertia of 277 Elvira give a value of around 190 J m⁻² K⁻¹ s^−1/2, compared to 50 for lunar regolith and 400 for coarse sand in an atmosphere.^[2]

References

↑ ^1.0 ^1.1 ^1.2 ^1.3 "277 Elvira". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=277;cad=1.
↑ ^2.0 ^2.1 ^2.2 ^2.3 Delbo', Marco; Tanga, Paolo (February 2009), "Thermal inertia of main belt asteroids smaller than 100 km from IRAS data", Planetary and Space Science 57 (2): pp. 259–265, doi:10.1016/j.pss.2008.06.015, Bibcode: 2009P&SS...57..259D.
↑ Schmadel Lutz D. Dictionary of Minor Planet Names (fifth edition), Springer, 2003. ISBN:3-540-00238-3.
↑ Slivan, S. M., Binzel, R. P., Crespo da Silva, L. D., Kaasalainen, M., Lyndaker, M. M., Krco, M.: "Spin vectors in the Koronis family: comprehensive results from two independent analyses of 213 rotation lightcurves",Icarus, 162, 2003, pp. 285–307.

External links

277 Elvira at AstDyS-2, Asteroids—Dynamic Site
- Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
277 Elvira at the JPL Small-Body Database
- Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

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Original source: https://en.wikipedia.org/wiki/277 Elvira. Read more

[jpldata-1] 1.0 ^1.1 ^1.2 ^1.3 "277 Elvira". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=277;cad=1.

[Delbo2009-2] 2.0 ^2.1 ^2.2 ^2.3 Delbo', Marco; Tanga, Paolo (February 2009), "Thermal inertia of main belt asteroids smaller than 100 km from IRAS data", Planetary and Space Science 57 (2): pp. 259–265, doi:10.1016/j.pss.2008.06.015, Bibcode: 2009P&SS...57..259D.

[3] Schmadel Lutz D. Dictionary of Minor Planet Names (fifth edition), Springer, 2003. ISBN:3-540-00238-3.

[4] Slivan, S. M., Binzel, R. P., Crespo da Silva, L. D., Kaasalainen, M., Lyndaker, M. M., Krco, M.: "Spin vectors in the Koronis family: comprehensive results from two independent analyses of 213 rotation lightcurves",Icarus, 162, 2003, pp. 285–307.

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277 Elvira

Topic: Astronomy

References

External links