{
 "id": "ep0g12781j",
 "slug": "5511-cloanthus",
 "title": "5511 Cloanthus",
 "updated": "2026-10-25",
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 "excerpt": "5511 Cloanthus is a large Jupiter Trojan asteroid about 40 kilometers wide with a slow, tumbling 336-hour rotation, never coming near Earth's orbit and not classified as potentially hazardous.",
 "snippet": "5511 Cloanthus is a large Jupiter Trojan asteroid about 40 kilometers wide with a slow, tumbling 336-hour rotation, never coming near Earth's orbit and not classified as potentially hazardous.",
 "node": "places.extraterrestrial.small-bodies.asteroids-trojans-and-outer-groups.trojan-camp-jupiter-trojans",
 "markdown": "# 5511 Cloanthus\n\n**5511 Cloanthus** (provisional designation 1988 TH1) is a large Jupiter Trojan asteroid, one of the bodies trapped in a 1:1 mean-motion resonance with Jupiter near its L4 and L5 Lagrangian points.\n\n| Key fact | Detail |\n|---|---|\n| Orbit | Semi-major axis 5.255 AU, eccentricity 0.119, inclination 11.17°; period 4,400 days (12.05 years)<sup>[1](https://www.spacereference.org/asteroid/5511-cloanthus-1988-th1)</sup> |\n| Distance range | Perihelion 4.63 AU, aphelion 5.88 AU from the Sun<sup>[1](https://www.spacereference.org/asteroid/5511-cloanthus-1988-th1)</sup> |\n| Rotation | 336.00 hours per revolution, a slow, tumbling (non-principal-axis) rotation<sup>[2](https://iaaras.ru/html/emp2021/emp_2021/parcur21d.pdf)</sup> |\n| Hazard status | Not a near-Earth object and not classified as potentially hazardous; its orbit stays 3.63 AU from Earth's orbit at the closest point<sup>[1](https://www.spacereference.org/asteroid/5511-cloanthus-1988-th1)</sup> |\n\n## Orbit and dynamical setting\n\n[Jupiter Trojans](https://www.edgepedia.org/jupiter-trojans) follow essentially the same orbit as Jupiter, leading or trailing the planet by about 60 degrees in co-orbital motion.<sup>[3](https://www.nature.com/articles/nature03540)</sup> Cloanthus fits this pattern with a semi-major axis of 5.255 AU, close to Jupiter's own 5.2 AU, and an orbital period of 4,400 days, or 12.05 years.<sup>[1](https://www.spacereference.org/asteroid/5511-cloanthus-1988-th1)</sup> Its eccentricity of 0.119 carries it from 4.63 AU at perihelion to 5.88 AU at aphelion, and its orbit is inclined 11.17 degrees to the ecliptic.<sup>[1](https://www.spacereference.org/asteroid/5511-cloanthus-1988-th1)</sup>\n\nThe orbit is well determined. Observations used for its orbit solution extend back to a precovery from July 30, 1951, and the [Minor Planet Center](https://www.edgepedia.org/minor-planet-center) records 3,135 observations, with the last official observation on July 3, 2023.<sup>[1](https://www.spacereference.org/asteroid/5511-cloanthus-1988-th1)</sup> A Czech astronomical database lists 4,831 observations across 35 oppositions, observed from 1951 onward.<sup>[4](https://astronomia.zcu.cz/planety/planetka-5511)</sup>\n\nBecause the orbit never approaches [Earth's orbit](https://www.edgepedia.org/earths-orbit) closer than 3.63 AU, JPL's CNEOS simulations show no close approaches, and the asteroid is not classified as potentially hazardous. It is also not considered a viable target for human exploration by the NHATS study.<sup>[1](https://www.spacereference.org/asteroid/5511-cloanthus-1988-th1)</sup>\n\n## Physical properties\n\nThe two estimates bracket the true size, which depends on how reflective the surface actually is.\n\nRotation is unusually slow. Photometric monitoring gives a rotation period of 336.00 hours, about 14 Earth days, and the asteroid is cataloged as a tumbling body rotating in non-principal-axis rotation rather than about a single fixed axis.<sup>[2](https://iaaras.ru/html/emp2021/emp_2021/parcur21d.pdf)</sup><sup> • </sup><sup>[1](https://www.spacereference.org/asteroid/5511-cloanthus-1988-th1)</sup> Slow, complex rotation of this kind is found among a subset of larger asteroids and is consistent with the long rotation periods reported for many Jupiter Trojans.<sup>[5](https://doi.org/10.1007/s11214-024-01052-7)</sup>\n\nTrojans as a population are thought to be more primitive than main-belt asteroids, believed to have formed at a range of heliocentric distances in the trans-Neptunian region, been scattered inward, and been captured during giant planet migration.<sup>[5](https://doi.org/10.1007/s11214-024-01052-7)</sup> Cloanthus shares this origin story with the rest of the Trojan clouds.\n\n## Occultations and observation opportunities\n\nBecause Cloanthus is large and its orbit is well known, it occasionally occults background stars. On 2019 May 3 UT, the roughly 40 km asteroid occulted a magnitude 12.1 star in the constellation Virgo for observers along a narrow path across northern [Queensland](https://www.edgepedia.org/queensland) and the Northern Territory of Australia; at that time the asteroid was 4.41 AU from Earth.<sup>[6](https://www.occultations.org.nz/planet/2019/updates/190503_5511_59986_u.htm)</sup> Stellar occultations by Trojans are used to constrain sizes and shapes beyond what photometry alone provides.\n\n## References\n\n1. [Asteroid Cloanthus (5511), Space Reference](https://www.spacereference.org/asteroid/5511-cloanthus-1988-th1)\n2. [Non-principal axis rotation (tumbling) asteroids table, IAA RAS](https://iaaras.ru/html/emp2021/emp_2021/parcur21d.pdf)\n3. [Morbidelli et al. (2005). Chaotic capture of Jupiter's Trojan asteroids in the early Solar System. Nature 435, 462–465.](https://www.nature.com/articles/nature03540)\n4. [Planetka Cloanthus (5511), Astronomia ZČU](https://astronomia.zcu.cz/planety/planetka-5511)\n5. [Mottola et al. (2024). Shapes, Rotations, Photometric and Internal Properties of Jupiter Trojans. Space Science Reviews 220, 17.](https://doi.org/10.1007/s11214-024-01052-7)\n6. [RASNZ Occultation Section: Cloanthus Occultation Update, 2019 May 3](https://www.occultations.org.nz/planet/2019/updates/190503_5511_59986_u.htm)\n\n---\n*Topic: Encyclopedia › Places and geography › Extraterrestrial places › Small bodies of the Solar System › Jupiter Trojans and other dynamical groups › Trojan-camp Jupiter Trojans*\n\n*Initially written Oct 21, 2026 · Edited: Oct 25, 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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 "markdown_url": "https://www.edgepedia.org/5511-cloanthus.md",
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 "credit": "\"5511 Cloanthus\", Edgepedia (EdgeChat), https://www.edgepedia.org/5511-cloanthus. Edgepedia Community License 1.0.",
 "credit_md": "\"[5511 Cloanthus](https://www.edgepedia.org/5511-cloanthus)\", Edgepedia (EdgeChat), [https://www.edgepedia.org/5511-cloanthus](https://www.edgepedia.org/5511-cloanthus). [Edgepedia Community License 1.0](https://www.edgepedia.org/edgepedia/license).",
 "credit_html": "\"<a href=\"https://www.edgepedia.org/5511-cloanthus\">5511 Cloanthus</a>\", Edgepedia (EdgeChat), <a href=\"https://www.edgepedia.org/5511-cloanthus\">https://www.edgepedia.org/5511-cloanthus</a>. <a href=\"https://www.edgepedia.org/edgepedia/license\">Edgepedia Community License 1.0</a>.",
 "speakable": "5511 Cloanthus is a large Jupiter Trojan asteroid about 40 kilometers wide with a slow, tumbling 336-hour rotation, never coming near Earth's orbit and not classified as potentially hazardous."
}
