Generated by DeepSeek V3.2| Lutetia | |
|---|---|
| Name | Lutetia |
| Caption | Image of Lutetia taken by the Rosetta spacecraft in 2010 |
| Discoverer | Hermann Goldschmidt |
| Discovery date | November 15, 1852 |
| Designation | 21 Lutetia |
| Mp category | Main belt asteroid |
| Epoch | July 14, 2004 |
| Semimajor | 2.435 AU |
| Perihelion | 2.037 AU |
| Aphelion | 2.833 AU |
| Eccentricity | 0.163 |
| Period | 3.80 yr |
| Inclination | 3.064° |
| Dimensions | 121±1 × 101±1 × 75±13 km |
| Mass | (1.700±0.017)×1018 kg |
| Density | 3.4±0.3 g/cm³ |
| Rotation period | 8.165455 h |
| Spectral type | M-type (Xk-type) |
| Abs magnitude | 7.29 |
| Albedo | 0.19±0.01 (geometric) |
Lutetia is a large asteroid located in the asteroid belt between the orbits of Mars and Jupiter. Discovered in 1852 by Hermann Goldschmidt from his balcony in Paris, it is named after the Latin name for the city of Paris. As one of the largest M-type asteroids, it has been the subject of significant scientific interest, culminating in a close flyby by the European Space Agency's Rosetta spacecraft in 2010, which revealed a complex, ancient, and cratered world.
The discovery of this asteroid was announced by Hermann Goldschmidt on November 15, 1852, following observations from his residence in the Latin Quarter of Paris. The name, proposed by François Arago, honors the city's Gallo-Roman heritage, linking it to the Parisii tribe. Its early observations were part of a broader effort by 19th century astronomers like Urbain Le Verrier to catalog minor planets. For over a century, it remained a point of light in telescopes, with its physical nature a mystery until the advent of space probes. The International Astronomical Union later officially designated it as asteroid number 21 Lutetia.
This body is an irregularly shaped object, with dimensions measured by Rosetta showing a triaxial ellipsoid structure. Its surface is dominated by a heavily cratered highland region known as the Achaia region, contrasting sharply with the smoother, younger Noricum region. A prominent feature is a large impact basin named Massilia, along with extensive systems of grooves, rilles, and landslide scars. The north polar region exhibits a thick blanket of regolith, while the equatorial areas show dramatic escarpments and boulder fields, indicating a long and violent geological history.
Data from Rosetta's instruments, including the OSIRIS imaging system and the VIRTIS spectrometer, revealed a surprisingly complex body. While classified as an M-type asteroid, its surface lacks the high metal content expected, showing instead a composition akin to enstatite chondrite or carbonaceous chondrite meteorites. The surface is covered with a primitive, unprocessed regolith, and spectral analysis suggests the presence of silicates, hydrated minerals, and possibly phyllosilicates. Its high density implies it may be a primordial, partially differentiated remnant from the early Solar System, potentially containing a metallic core overlain by a primitive mantle.
Prior to the Rosetta mission, knowledge came from ground-based telescope observations and measurements by the IRAS and Hubble. The defining moment was the July 10, 2010 flyby, when Rosetta passed within 3,162 km. The encounter, managed by the European Space Operations Centre, provided over 400 images and data from instruments like ALICE, MIRO, and CONSERT. This data transformed it from a point of light into a mapped world, with findings later analyzed by teams at the Max Planck Institute for Solar System Research and the Institut d'Astrophysique Spatiale.
As the namesake of Lutetia, the asteroid maintains a unique bond with the city of Paris. It has been referenced in works of science fiction, including the novel Le Rêve des Forêts by Maurice Renard. The Paris Observatory has historically featured its discovery in exhibitions. In a notable tribute, a Google Doodle on November 15, 2012 commemorated the 160th anniversary of its discovery by Hermann Goldschmidt. The data from the Rosetta mission continues to be a cornerstone for studies at institutions like NASA's Jet Propulsion Laboratory and the University of Paris.
Category:Asteroids Category:Asteroids visited by spacecraft Category:Named minor planets