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13 Egeria
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Main-belt asteroid
Egeria (disambiguation)Egeria
September 2025
yes #D6D6D6 13 Egeria 13 Egeria VLT (2021), deconvolved.pdf A deconvolved image of 13 Egeria by VLT/SPHERE 24px|class=skin-invert|alt=13 Egeria symbol| (historical)24px|class=skin-invert|alt=Original buckler symbol (variant) Annibale de Gasparis Naples Obs. 2 November 1850 ᵻ ˈ dʒ ɪər i əNoah Webster (1884) A Practical Dictionary of the English Language Egerian Egeria (13) Egeria 1850 VA Main belt 17.0 October 2024 (JD 2460600.5) 2.57774 AU 2.35759 AU 2.79788 AU 0.085403 4.14 yr (1511.7 d) 16.532° 43.208° 79.222° 305.547° 18.56 km/s 202 3 km207.6 ± 8.3 km (IRAS) 214.8 km × 192 km238 x 199 x 182 km (± 12 x 11 x 10 km) 0.24Flattening derived from the maximum aspect ratio (c/a): , where (c/a) = 0.76 0.06. 7.24 0.34 18 kgCalculated from its standard gravitational parameter GM = 0.483 0.023 km3 s2. 1.68 0.11 g/cm3Assuming a diameter of 202 ± 3 km. ≈0.0580 m/s2 ≈0.1098 km/s 7.045 h7.046664 0.000003 h 59° G-type asteroid 9.71 to 12.46apmag 9.71 (2061-Nov-06) to 12.46 (1990-Mar-12) JPL Horizons daily output for 1950 to 2099 6.916.74 31 5 deg 38 5 deg 0.0870.049 ± 0.0280.085 ± 0.007http://www.psi.edu/pds/archive/astdata04/simps04/diamalb.tab https://archive.today/20060523221500/http://www.psi.edu/pds/archive/astdata04/simps04/diamalb.tab dead 2006-05-23 Asteroid Data Archive 2008-11-03 Planetary Science Institute ~174 K 0.23815 ms / day 63566 days (174.03 yr) 0 1.43636 AU 2.35842 AU 3.363
13 Egeria is a large main-belt G-type asteroid. It was discovered by Annibale de Gasparis on 2 November 1850. Egeria was named by Urbain Le Verrier, whose computations led to the discovery of Neptune, after the mythological nymph Egeria of Aricia, Italy, the wife of Numa Pompilius, second king of Rome.
History
Egeria was discovered on the evening of 2 November 1850 by Italian astronomer Annibale de Gasparis at the Astronomical Observatory of Capodimonte.128 Whereas de Gasparis's previous two discoveries—10 Hygiea and 11 Parthenope—were identified by comparison with the Berlin Academy star charts, Egeria was identified using his own ecliptic charts intended for finding new celestial objects.119128 Egeria's discovery was announced in December 1850 by astronomer Benjamin A. Gould through The Astronomical Journal. Following the discovery, de Gasparis delegated the naming rights of the asteroid to Urbain Le Verrier. Le Verrier chose to name the asteroid after Egeria, a mythological nymph and councillor of Numa Pompilius.128
Upon its discovery, both de Gasparis and Gould labelled Egeria as a new planet. However, by the mid-1800s, the classification and terminology of the asteroids were quickly evolving. Soon after Egeria's discovery, other astronomers described it as an "asteroid" or a "minor planet".25 Throughout the latter half of the 19th century, the terms "asteroid" and "minor planet" became favored, although some publications continued to label Egeria and other asteroids as planets.42
In 1851, de Gasparis announced his chosen symbol for Egeria—that of a buckler. However, Gould had apparently not seen the announcement, and in an 1852 table of asteroid symbols he left Egeria's blank.8 No mention of a star was made, though in 1852 John Russell Hind included one in his drawn symbol for Egeria: 15px|class=skin-invert|alt=13 Egeria symbol (U+1CEC6 in Unicode 17.0). The symbol is sometimes depicted with a round form (15px|class=skin-invert|alt=Variant 13 Egeria symbol),8 though only Hind's form was encoded. Miscellaneous Symbols Supplement 2025 unicode.org The Unicode Consortium https://www.unicode.org/charts/PDF/U1CEC0.pdf September 9, 2025 live As the number of asteroids assigned a symbol grew in number through the mid-1800s, the practicality of assigning each a unique astronomical symbol was questioned. In 1851, astronomer Johann Franz Encke proposed an alternative system of a number—denoting the object's order of discovery—inscribed in a circle. For Egeria, this would be ⑬. This system was quickly adopted by astronomers, though eventually astronomers switched from an inscribed circle to parentheses and eventually a bare number—hence (13) Egeria or 13 Egeria in modern notation.
Orbit
Egeria orbits the Sun at an average distance—its semi-major axis—of 2.58 astronomical units (AU), placing it within the main asteroid belt and near the 3:1 mean-motion resonance with Jupiter.323 Along its orbit, its distance from the Sun varies between 2.36 AU at perihelion to 2.80 AU at aphelion due to its orbital eccentricity of 0.09. Its orbit is inclined by 16.5° with respect to the ecliptic, and it takes 4.14 years to complete one orbit. Egeria is classified as a background asteroid, as it does not belong to an asteroid family.
Physical properties
thumb|left|200px|OCCULT4 visualization of Egeria's 2008 occultation event
Egeria occulted a star on 8 January 1992. Its disc was determined to be quite circular (217×196 km). On 22 January 2008, it occulted another star, and this occultation was timed by several observers in New Mexico and Arizona, coordinated by the IOTA Asteroid Occultation Program. The result showed that Egeria presented an approximately circular profile to Earth of 214.8×192 km, well in agreement with the 1992 occultation.April 2014 It has also been studied by radar.
In 1988 a search for satellites or dust orbiting this asteroid was performed using the UH88 telescope at the Mauna Kea Observatories, but the effort came up empty. Spectral analysis of Egeria shows it to be unusually high in water content, 10.5–11.5% water by mass.
thumb|A three-dimensional model of 13 Egeria based on its light curve
See also
Former classification of planets
Notes
References
(13) Egeria = 1850 VA
https://www.minorplanetcenter.net/db_search/show_object?utf8=%E2%9C%93&object_id=13
Minor Planet Center
8 September 2025
2024-12-04 last obs
JPL Small-Body Database Browser: 13 Egeria
http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=13
21 December 2024
(13) Egeria – Proper Elements
https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=13
Asteroids Dynamic Site
24 January 2026
Vernazza P.
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Astronomy and Astrophysics
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A56
10.1051/0004-6361/202141781
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10045/118969
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Gavin Jared Bala
Kirk Miller
Unicode request for historical asteroid symbols
https://www.unicode.org/L2/L2023/23207-historical-asteroids.pdf
18 September 2023
unicode.org
Unicode
26 September 2023
The Solar System: Descriptive Treatise Upon the Sun, Moon, and Planets, Including an Account of All the Recent Discoveries
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Chapter VIII. The Minor or Ultra-Zodiacal Planets.
https://archive.org/details/solarsystemdescr00hind/page/126/mode/2up
John Russell Hind
John Russell Hind
1852
126
G. P. Putnam's Sons
New York, United States
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http://www.asteroidoccultation.com/observations/Results/Data2008/20080122_EgeriaProfile.png IOTA Asteroid Occultation Results for 2008 Timerson Brad 2010-01-19 https://web.archive.org/web/20140416210320/http://www.asteroidoccultation.com/observations/Results/Data2008/20080122_EgeriaProfile.png 2014-04-16 dead
Schmadel Lutz D. Dictionary of minor planet names 1 5th 2003 Springer-Verlag Berlin Heidelberg New York 3-540-00238-3 16
http://www.lpi.usra.edu/meetings/LPSC98/pdf/1310.pdf High-resolution 2.5–3.5 M Observations of C-, B- and G-class asteroids. Rivkin A. S. J. K. Davies S. L. Ellison L. A. Lebofsky 2008-04-20
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Fuentes-Muñoz Oscar Farnocchia Davide Giorgini Jon D. Park Ryan S. 2025-12-01 Asteroid Mass Estimation by Mutual Perturbations During Close Encounters After Gaia Focused Product Release The Astronomical Journal 170 6 353 10.3847/1538-3881/ae0cc9 0004-6256 free 2025AJ....170..353F 283347135
External links
Elements and Ephemeris for (13) Egeria Minor Planet Center http://scully.cfa.harvard.edu/cgi-bin/returnprepeph.cgi?d=b2011&o=00013 dead https://web.archive.org/web/20160304084942/http://scully.cfa.harvard.edu/cgi-bin/returnprepeph.cgi?d=b2011&o=00013 2016-03-04 2011-05-26 (displays Elong from Sun and V mag for 2011)
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