What Is 11 Per

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Last updated: April 14, 2026

Quick Answer: 11 Per refers to the asteroid 11 Parthenope, discovered on May 11, 1850, by Annibale de Gasparis. It has a diameter of approximately 153 kilometers and orbits the Sun every 4.8 years. The asteroid is part of the main belt between Mars and Jupiter and is named after Parthenope, a figure in Greek mythology. It rotates once every 13.7 hours and is composed primarily of silicate rock.

Key Facts

Overview

The celestial object known as 11 Parthenope is a large main-belt asteroid orbiting the Sun between Mars and Jupiter. It was the 11th asteroid ever discovered, hence its numerical designation, and was identified on May 11, 1850, by the Italian astronomer Annibale de Gasparis at the Capodimonte Observatory in Naples, Italy. This discovery marked a significant milestone in 19th-century astronomy, contributing to the growing understanding of minor planets in our solar system.

Named after Parthenope, a Siren from Greek mythology who was said to be the daughter of the river god Achelous and the muse Calliope, the asteroid reflects the tradition of naming celestial bodies after figures from classical mythology. Parthenope, in legend, was believed to have drowned after failing to charm Odysseus with her song and was later buried in what is now Naples, linking the name to the region where it was discovered. This mythological connection adds cultural and historical depth to the scientific significance of the object.

11 Parthenope is classified as an S-type asteroid, indicating a silicate-rich composition, which is common among inner-belt asteroids. Its discovery helped expand the catalog of known asteroids during a period of rapid astronomical advancement in Europe. As one of the earlier-found asteroids, it played a role in shaping early models of the solar system’s structure and continues to be studied for insights into the formation and evolution of the asteroid belt.

How It Works

Understanding 11 Parthenope involves examining its physical and orbital mechanics, which govern how it moves and interacts within the solar system. As a member of the main asteroid belt, it follows an elliptical orbit influenced by the gravitational forces of the Sun and nearby planets, particularly Jupiter. Scientists study its light curves, spectral data, and trajectory to determine characteristics such as rotation, composition, and potential for future exploration.

Key Details and Comparisons

AsteroidDiameter (km)Orbital Period (years)Rotation Period (hours)Discovery YearType
11 Parthenope1534.813.71850S-type
1 Ceres9394.69.11801P-type
4 Vesta5253.65.31807V-type
2 Pallas5124.67.81802B-type
433 Eros16.81.85.31898S-type

The comparison above highlights how 11 Parthenope fits within the broader context of asteroid discoveries. While significantly smaller than the largest asteroids like Ceres and Vesta, it is still substantial in size compared to near-Earth objects like 433 Eros. Its 4.8-year orbital period is typical for main-belt asteroids located at around 2.5 AU from the Sun. Unlike Ceres, which is now classified as a dwarf planet, Parthenope remains a standard asteroid with no planetary status. Its S-type classification aligns it with stony bodies that are more common in the inner asteroid belt, distinguishing it from carbon-rich C-types found farther out. These comparisons help astronomers categorize and prioritize targets for observation and potential space missions.

Real-World Examples

11 Parthenope has been observed in numerous astronomical surveys and has contributed to scientific research on asteroid composition and dynamics. For instance, data from NASA’s Infrared Astronomical Satellite (IRAS) helped refine estimates of its size and albedo. Additionally, ground-based telescopes equipped with spectrographs have analyzed its surface materials, confirming the presence of silicate minerals consistent with S-type classification. These observations are critical for understanding the distribution of materials in the early solar system.

While not a target of any dedicated space mission, 11 Parthenope has been included in broader asteroid studies and cataloging efforts. Its orbit is well-documented by the Minor Planet Center, and its trajectory is regularly updated to ensure accuracy in celestial navigation databases. The asteroid serves as a reference point for testing models of orbital perturbations caused by Jupiter’s gravity.

  1. IRAS Observations: Provided thermal data used to calculate diameter and surface properties.
  2. Light Curve Studies: Conducted by amateur and professional astronomers to determine rotation period.
  3. Spectral Analysis: Performed at observatories to confirm silicate-rich composition.
  4. Orbital Tracking: Ongoing monitoring by the Minor Planet Center for accuracy in ephemerides.

Why It Matters

11 Parthenope, though not widely known outside astronomical circles, plays an important role in advancing our understanding of the solar system’s formation and the nature of minor planets. Its discovery in the mid-19th century was part of a wave of astronomical progress that laid the foundation for modern planetary science. Continued study of asteroids like Parthenope helps scientists refine models of accretion, collisional evolution, and space weathering.

As humanity expands its reach into space, asteroids like 11 Parthenope may become targets for future robotic exploration or even resource utilization. Their study not only enriches our knowledge of planetary science but also prepares us for the challenges and opportunities of deep space exploration. In this way, even lesser-known celestial bodies contribute meaningfully to the broader quest to understand our place in the cosmos.

Sources

  1. WikipediaCC-BY-SA-4.0

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