What Is 11506 Toulouse-Lautrec
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Last updated: April 14, 2026
Key Facts
- Discovered on December 18, 1981
- Discovered by Schelte J. Bus at Siding Spring Observatory
- Named after Henri de Toulouse-Lautrec, French artist
- Orbital period of 4.37 years
- Semi-major axis of 2.63 AU
- Member of the Eos asteroid family
- Designated minor planet number 11506
Overview
11506 Toulouse-Lautrec is a main-belt asteroid located between Mars and Jupiter, designated by the Minor Planet Center with the number 11506. It was discovered on December 18, 1981, by American astronomer Schelte J. Bus during a sky survey conducted at the Siding Spring Observatory in New South Wales, Australia. This observatory, part of the Australian National University, has been instrumental in identifying thousands of minor planets due to its location in the Southern Hemisphere and access to advanced telescopic equipment.
The asteroid was originally cataloged as 1981 YP1—a provisional designation based on the year and timing of its discovery—before receiving its permanent number and name. The naming of celestial bodies often honors notable figures in science, culture, and history, and in this case, 11506 Toulouse-Lautrec pays tribute to Henri de Toulouse-Lautrec, the French painter and illustrator famed for his iconic posters and scenes of Parisian cabarets like the Moulin Rouge in the 1890s. His work bridged the gap between fine art and popular culture, making him a fitting namesake for an object in the vast cultural expanse of the solar system.
The significance of naming asteroids after cultural icons lies in the tradition of commemorating human achievement through astronomical discovery. By naming this asteroid after Toulouse-Lautrec, the International Astronomical Union (IAU) recognizes the enduring legacy of art in human civilization. With an estimated diameter of around 10 to 20 kilometers, 11506 Toulouse-Lautrec is relatively small compared to larger asteroids like Ceres or Vesta, but its classification within the Eos family provides valuable insights into the collisional history of the asteroid belt.
How It Works
Understanding how 11506 Toulouse-Lautrec functions within the solar system involves examining its orbital mechanics, physical characteristics, and classification. As a main-belt asteroid, it follows a predictable elliptical path around the Sun governed by gravitational forces. Its motion is studied using astrometric tracking, photometric analysis, and spectral classification to determine composition and origin.
- Orbital Period: The asteroid completes one orbit around the Sun every 4.37 years, or approximately 1,596 days. This period places it firmly within the central region of the asteroid belt.
- Semi-Major Axis: With a semi-major axis of 2.63 astronomical units (AU), it orbits at an average distance of about 393 million kilometers from the Sun, placing it between Mars and Jupiter.
- Orbital Eccentricity: Its orbit has an eccentricity of 0.11, meaning it is slightly elliptical but not highly elongated.
- Inclination: The orbital plane is tilted at 10.8 degrees relative to the ecliptic, which is typical for members of the Eos family.
- Albedo: Estimated albedo is around 0.15, indicating a moderately reflective surface, likely composed of silicate-rich materials.
- Rotation Period: While not precisely measured, similar Eos family members have rotation periods between 4 to 12 hours, suggesting a likely range for 11506 Toulouse-Lautrec.
Key Details and Comparisons
| Asteroid | Discovery Year | Orbital Period (years) | Semi-Major Axis (AU) | Family |
|---|---|---|---|---|
| 11506 Toulouse-Lautrec | 1981 | 4.37 | 2.63 | Eos |
| 22 Kalliope | 1852 | 4.61 | 2.91 | None (individual) |
| 31 Euphrosyne | 1854 | 5.57 | 3.15 | Euphrosyn |
| 221 Eos | 1882 | 4.48 | 2.99 | Eos |
| 1 Ceres | 1801 | 4.61 | 2.77 | None (dwarf planet) |
The comparison highlights how 11506 Toulouse-Lautrec fits within the broader context of asteroid taxonomy and orbital dynamics. While it shares orbital similarities with 221 Eos, the parent body of its family, it is much smaller and less massive. Unlike 1 Ceres, which is classified as a dwarf planet and accounts for about 25% of the asteroid belt’s total mass, 11506 Toulouse-Lautrec is a minor fragment among millions. Its membership in the Eos family—a group of over 4,000 asteroids believed to have originated from a catastrophic collision over a billion years ago—links it to a shared mineralogical and dynamical history. Spectral analysis suggests these asteroids are predominantly K-type, indicating a composition rich in silicates and low in carbon, distinguishing them from darker C-type asteroids.
Real-World Examples
The naming of asteroids after artists is not unique to Toulouse-Lautrec. The IAU maintains strict guidelines for naming minor planets, often requiring discoverers to propose names that honor individuals who have made significant contributions to the arts, sciences, and humanities. For example, 1035 Amata is named after an Italian poet, and 2309 Mr. Spock—though controversial—was named after the astronomer’s cat. These names add a human dimension to the otherwise technical cataloging of celestial bodies.
Several asteroids have been named after figures in the visual arts, reinforcing the connection between creativity and discovery. Notable examples include:
- 9944 Brontë – Named after the Brontë sisters, renowned English novelists.
- 16037 Johnbarber – Honors a sculptor and educator.
- 17473 Franklloydwright – Named after the iconic American architect.
- 2001 Einstein – Honors physicist Albert Einstein, showing the breadth of cultural tribute.
Why It Matters
The study of asteroids like 11506 Toulouse-Lautrec contributes to our understanding of solar system formation, planetary defense, and the origins of materials found on Earth. Each asteroid serves as a time capsule preserving conditions from the early solar system, offering clues about planetary accretion and collisional evolution.
- Impact: Provides data on the composition and distribution of the Eos family, helping model ancient collisions in the asteroid belt.
- Scientific Value: Offers insights into the mineralogy of K-type asteroids, which may differ from more common C- or S-types.
- Cultural Significance: Bridges science and art by honoring influential cultural figures in astronomical nomenclature.
- Educational Role: Serves as a teaching tool in astronomy courses to illustrate asteroid classification and naming conventions.
- Discovery Legacy: Highlights the contributions of Schelte J. Bus, who discovered over 1,700 asteroids during his career.
Ultimately, 11506 Toulouse-Lautrec exemplifies how science and culture intersect in modern astronomy. While it may never be visited by spacecraft, its name ensures that the legacy of Henri de Toulouse-Lautrec continues to inspire across disciplines—from the cabarets of 19th-century Paris to the cold, dark reaches of the asteroid belt.
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