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 "slug": "806-gyldenia",
 "title": "806 Gyldenia",
 "updated": "2026-10-21",
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 "excerpt": "806 Gyldenia (1915 WX), outer main-belt carbonaceous asteroid discovered 18 April 1915 by Max Wolf at Heidelberg; about 63-83 km across, albedo ~0.023, rotation period ~16.85 h, pole λ=235°, β=42°.",
 "snippet": "806 Gyldenia (1915 WX), outer main-belt carbonaceous asteroid discovered 18 April 1915 by Max Wolf at Heidelberg; about 63-83 km across, albedo ~0.023, rotation period ~16.85 h, pole λ=235°, β=42°.",
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 "markdown": "# 806 Gyldenia\n\n**806 Gyldenia** (provisional designation 1915 WX) is a carbonaceous asteroid in the outer region of the main asteroid belt, roughly 63 to 83 kilometers across depending on the measurement, with a very dark surface and a slow rotation period of about 16.85 hours. It was discovered on 18 April 1915 by the German astronomer [Max Wolf](https://www.edgepedia.org/max-wolf) at Heidelberg Observatory.<sup>[1](https://clever-geek.imtqy.com/articles/1389730/index.html)</sup>\n\n| Key fact | Detail |\n|---|---|\n| Discovery | 18 April 1915, Heidelberg, by Max Wolf; provisional designation 1915 WX<sup>[1](https://clever-geek.imtqy.com/articles/1389730/index.html)</sup> |\n| Orbit | Semi-major axis 3.204 AU, eccentricity 0.0812, inclination 14.22°, orbital period 2,100 days (5.75 years)<sup>[2](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)</sup> |\n| Diameter | Published estimates include 62.6 km<sup>[3](https://www.bahnsen.de/jens/astro/aster/h-gurt500-1000.htm)</sup> and 83.10 km<sup>[2](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)</sup>; the DAMIT shape model gives a calibrated 55 ± 4 km<sup>[4](https://damit.cuni.cz/asteroid_models/view/3880)</sup> |\n| Albedo | About 0.023, a very dark surface<sup>[2](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)</sup> |\n| Rotation | About 16.85 hours; the DAMIT model lists P = 16.857 h<sup>[4](https://damit.cuni.cz/asteroid_models/view/3880)</sup> |\n| Spin axis | Ecliptic pole coordinates λ = 235°, β = 42° in DAMIT model 3880<sup>[4](https://damit.cuni.cz/asteroid_models/view/3880)</sup> |\n| Observational record | 6,777 observations used for orbit determination, dating back to the 1915 discovery<sup>[2](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)</sup> |\n\n## Orbit and classification\n\nGyldenia orbits the Sun in the outer main belt between Mars and Jupiter, on a nearly circular path with eccentricity 0.0812 tilted 14.22° to the ecliptic. It comes as close as 2.94 AU and recedes to 3.46 AU, completing one revolution every 2,100 days at an average orbital speed of 16.60 km/s.<sup>[2](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)</sup> A German-language asteroid catalog lists a semi-major axis of 3.213 AU and a diameter of 62.6 km for the object.<sup>[3](https://www.bahnsen.de/jens/astro/aster/h-gurt500-1000.htm)</sup>\n\nThe asteroid is classified as an outer main-belt object and is not a near-Earth object. Its orbit stays at least 1.98 AU from [Earth's orbit](https://www.edgepedia.org/earths-orbit) at the closest point, and orbital simulations by NASA JPL's Center for Near-Earth Object Studies show no close approaches to Earth; it is also not rated a viable target for human exploration in the NHATS study.<sup>[2](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)</sup>\n\n## Size and surface\n\nDiameter estimates for Gyldenia differ by method. The value of 83.10 km comes from one survey determination and would make the asteroid larger than 99% of known asteroids, comparable in size to the U.S. state of Delaware.<sup>[2](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)</sup> Smaller values near 62.6 km appear in other compilations.<sup>[3](https://www.bahnsen.de/jens/astro/aster/h-gurt500-1000.htm)</sup> The shape model in the Database of Asteroid Models from Inversion Techniques (DAMIT), calibrated against size data, gives a volume-equivalent diameter of 55 ± 4 km.<sup>[4](https://damit.cuni.cz/asteroid_models/view/3880)</sup>\n\nAll determinations agree that the surface is very dark, with a geometric albedo of about 0.023, meaning the body reflects only a few percent of the sunlight hitting it. Such low albedos are typical of carbonaceous (C-type) asteroids in the outer belt.<sup>[2](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)</sup>\n\n## Rotation and shape model\n\nGyldenia is a slow rotator. Photometric campaigns have produced composite light curves from observing seasons in 2013, 2015, 2016, 2018, 2020, and 2021, with derived [synodic periods](https://www.edgepedia.org/synodic-period) clustered around 16.85 hours (for example 16.863 h in 2015, 16.857 h in 2018, and 16.853 h in 2021).<sup>[5](https://www.aanda.org/articles/aa/pdf/2023/11/aa46191-23.pdf)</sup> The DAMIT entry for the asteroid lists a sidereal period of 16.857 hours.<sup>[4](https://damit.cuni.cz/asteroid_models/view/3880)</sup>\n\nThe DAMIT shape model 3880, created in 2019 and last modified in October 2023, gives a spin-axis orientation of ecliptic longitude λ = 235° and latitude β = 42°, carries a quality flag of 3.5, and is a convex (non-nonconvex) model fitted with a Lambert-like light scattering law.<sup>[4](https://damit.cuni.cz/asteroid_models/view/3880)</sup> A 2023 study that scaled slowly rotating asteroids using stellar occultations reports that the spin solution for Gyldenia is constrained to within a few degrees.<sup>[6](https://www.researchgate.net/publication/374311646_Scaling_slowly_rotating_asteroids_with_stellar_occultations)</sup>\n\n## Observational history\n\nThe discovery observation of 18 April 1915 is the earliest data point in the object's record, and the [Minor Planet Center](https://www.edgepedia.org/minor-planet-center)'s orbit solution rests on 6,777 observations, with the most recent official observation recorded on 21 April 2023.<sup>[2](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)</sup> The DAMIT database holds dozens of individual light curves of Gyldenia, numbered 30745 through 30807, contributed to the shape-modeling effort.<sup>[7](https://damit.cuni.cz/projects/damit/asteroids/view/2202)</sup>\n\n## References\n\n1. [Asteroid List (801–900)](https://clever-geek.imtqy.com/articles/1389730/index.html)\n2. [Asteroid Gyldenia, Space Reference](https://www.spacereference.org/asteroid/806-gyldenia-a915-he)\n3. [Asteroiden des Hauptgürtels (500–1000)](https://www.bahnsen.de/jens/astro/aster/h-gurt500-1000.htm)\n4. [(806) Gyldenia – Model 3880, DAMIT](https://damit.cuni.cz/asteroid_models/view/3880)\n5. [Marciniak, A., et al. (2023). Scaling slowly rotating asteroids with stellar occultations. A&A, 679, A60](https://www.aanda.org/articles/aa/pdf/2023/11/aa46191-23.pdf)\n6. [Scaling slowly rotating asteroids with stellar occultations, ResearchGate](https://www.researchgate.net/publication/374311646_Scaling_slowly_rotating_asteroids_with_stellar_occultations)\n7. [Asteroid (806) Gyldenia, DAMIT](https://damit.cuni.cz/projects/damit/asteroids/view/2202)\n\n---\n*Topic: Encyclopedia › Places and geography › Extraterrestrial places › Small bodies of the Solar System › Main-belt asteroids and numbered minor planets › Outer-belt asteroids › Asteroids named after people*\n\n*Initially written Oct 21, 2026*\n\n*Copyright 2026 EdgeChat AI, a subsidiary of Biostate AI.*\n\nLicense: Edgepedia Community License 1.0, https://www.edgepedia.org/edgepedia/license\n",
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 "credit": "\"806 Gyldenia\", Edgepedia (EdgeChat), https://www.edgepedia.org/806-gyldenia. Edgepedia Community License 1.0.",
 "credit_md": "\"[806 Gyldenia](https://www.edgepedia.org/806-gyldenia)\", Edgepedia (EdgeChat), [https://www.edgepedia.org/806-gyldenia](https://www.edgepedia.org/806-gyldenia). [Edgepedia Community License 1.0](https://www.edgepedia.org/edgepedia/license).",
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 "speakable": "806 Gyldenia, outer main-belt carbonaceous asteroid discovered 18 April 1915 by Max Wolf at Heidelberg; about 63-83 km across, albedo ~0.023, rotation period ~16.85 h, pole λ=235°, β=42°."
}
