Metal Asteroids: Dense Rarities
![]() |
Illustration of 16 Psyche by Peter Rubin. Credit: NASA/JPL-Caltech/ASU |
Most asteroids are rocky debris from the formation of the solar system. However, some asteroids contain large amounts of metal, though they are generally much more rare, with only 38 asteroids known to date. These asteroids are likely the parent bodies for many meteorites, as metal tends to survive the heat of atmospheric entry better than rock.
These "M-type" asteroids will likely be important targets for future space mining opperations. Until then, let's take a look at some of the largest of these metal rich wonders.
16 Psyche
![]() |
Animation stills of topological features on Psyche. Credit: Shepard et al/CC BY-SA 4.0 |
- Date Discovered: March 17, 1852
- Designation: 16 Psyche (A852 FA)
- Mass: 2.29x10^19 Kilograms
- Radius: 111.5 Kilometres
- Density: 3.977 g/cm^3
- Rotational Period: 4.2 Hours
- Orbital Period: 1825.95 Days (4.999 Years)
- Moons: None
16 Psyche is the only M-type asteroid that is getting its own dedicated mission. Launching this October, NASA's Psyche spacecraft will enter orbit around the asteroid in 2029. Psyche was discovered by Annibale de Gasparis in 1852, Making it one of the first asteroids discovered. In fact, the "16" in Psyche's designation refers to the fact that was the sixteenth asteroid discovered. It is quite massive, and makes up 5% of the Asteroid Belt's mass. It was once thought to be the exposed core of a protoplanet, but new studies seem to refute this. However, NASA coverage of the mission seems to still refer to Psyche as a possible core, so perhaps we just won't know for sure until the Psyche spacecraft gets there.
21 Lutetia
![]() | |
|
- Date Discovered: November 15, 1852
- Designation: 21 Lutetia (A852 VA)
- Mass: 1.7x10^18 Kilograms
- Radius: 47.88 Kilometres
- Density: 3.45 g/cm^3
- Rotational Period: 8.17 Hours
- Orbital Period: 1388.49 Days (3.8 Years)
- Moons: None
Lutetia is a large main belt asteroid that was imaged by the Rosetta spacecraft on its way to comet 67P. Lutetia remains the only M-type asteroid to be visited by a spacecraft, until Psyche reaches its target. Lutetia was named after the Latin name for Paris, by it's discoverer; Hermann Goldschmidt. Lutetia is a relatively sterotypical looking asteroid, with an irregular shape, and many impact craters. When Rosetta flew by the asteroid in 2010, it imaged half its surface at a resolution of around 60 meters per pixel. While Lutetia is an M-type asteroid, its metal content is more of a coating, and doesn't make up the bulk of the asteroid's mass.
22 Kalliope
![]() |
Image of Kalliope from VLT. Credit: ESO/Vernazza et al/MISTRAL algorithm (ONERA/CNRS) CC BY 4.0 |
- Date Discovered: November 16, 1852
- Designation: 22 Kalliope (A852 WA)
- Mass: 2.29x10^19 Kilograms
- Radius: 83.77 Kilometres
- Density: 2.37 g/cm^3
- Rotational Period: -4.15 Hours*
- Orbital Period: 1814.29 Days (4.97 Years)
- Moons: 1 (Linus)
![]() |
Hesperia shape model. Credit: Astronomical Institute of the Charles University: Josef Durech, Vojtech Sidorin |
- Date Discovered: April 29, 1861
- Designation: 69 Hesperia (A861 HC)
- Mass: 5.86x10^18 Kilograms
- Radius: 69.065 Kilometres
- Density: 4.38 g/cm^3
- Rotational Period: 5.66 Hours
- Orbital Period: 1875.1 Days (5.13 Years)
- Moons: None
Hesperia was discovered by Giovanni Schiaparelli in 1861, while he was looking for asteroid 63 Ausonia. The asteroid is named after Schiaparelli's home nation of Italy, with Hesperia meaning peninsula in Greek. The spectra of this asteroid resembles that of the famous Hoba meteorite, the largest meteorite found on Earth to date.
92 Undina
![]() |
Undina's orbit. Credit: Solar System Dynamics |
- Date Discovered: July 7, 1867
- Designation: 92 Undina (A867 NA)
- Mass: 4.43x10^18 Kilograms
- Radius: 63.21 Kilometres
- Density: 4.39 g/cm^3
- Rotational Period: -15.94 Hours*
- Orbital Period: 2076.14 Days (5.68 Years)
- Moons: None
![]() |
Antigon shape model. Credit: Astronomical Institute of the Charles University: Josef Durech, Vojtech Sidorin |
- Date Discovered: February 5, 1873
- Designation: 129 Antigone (A873 CA)
- Mass: 2.65x10^18 Kilograms
- Radius: 56.5 Kilometres
- Density: 2.96 g/cm^3
- Rotational Period: 4.96 Hours
- Orbital Period: 1773.5 Days (4.86 Years)
- Moons: Tentative Satellite
Unlike some of the other asteroids in this article, Antigon is believed to be much more pure in its metallic composition. In fact, it could be quite similar to Psyche, but on a smaller scale.
216 Kleopatra
![]() |
Kleopatra model and faint images of its two moons. Credit: ESO/Vernazza, Marchis et al./MISTRAL algorithm (ONERA/CNRS) |
- Date Discovered: April 10, 1880
- Designation: 216 Kleopatra (A880 GB)
- Mass: 2.65x10^18 Kilograms
- Radius: 61 Kilometres (Average)
- Density: 3.45 g/cm^3
- Rotational Period: 5.39 Hours
- Orbital Period: 1705.07 Days (4.67 Years)
- Moons: 2 (Alexhelios & Cleoselene)
Comments
Post a Comment