Asteroid 216 Kleopatra
November 1, 2021
Wheat and
peanuts are
crops that are easily
cultivated and
harvested. For those reasons, these are
inexpensive food ingredients that are used in many
supermarket items. That's bad news for the many people with
peanut allergy or
gluten intolerance, who need to carefully read
product ingredient labels. These ubiquitous crops are the subject of many
cultural memes, as in the
adage, "
Man does not live by bread alone."
Economists assert that some people are willing to "
work for peanuts."
There's also the
Charles M.Schulz (1922-2000) comic strip,
Peanuts, and the
foam peanut packaging material, now mostly displaced by the
bubble wrap successor,
polyethylene bags filled with
air. The peanut is
personified in the
character,
Mr. Peanut, used as the
advertising logo and
mascot of
Planters for more than a
century. Mr. Peanut reportedly is
named, Bartholomew Richard Fitzgerald-Smythe, which sounds like the name of a character on one of the many
British television series on
PBS.
The peanut plant, Arachis hypogaea.
The peanut is an Angiosperm (lowering plant). The name derives from the Greek, angeion (αγγείον, vessel) and sperma (σπέρμα, seed) In the peanut case, the vessel is its shell.
The peanut is the most commercially important member of the seventy member genus, Arachis. As befits its name, the peanut is in the pea family (Fabaceae).
(An 1887 image by Franz Eugen Köhler from Köhler's Medizinal-Pflanzen, via Wikimedia Commons. Click for larger image.)
A peanut's
shape is a consequence of its being a
dicotyledon, the name given to
plants having
seeds with two elements. Since this shape is generally recognized, some items are designated as peanut-shaped. One of these is the
minor planet,
(486958) 2014 MU69, also known as Ultima Thule, discovered in 2014 by the
Hubble Space Telescope. I wrote about Ultima Thule in an
earlier article (Ultima Thule, January 7, 2019).
Image of Ultima Thule, (486958) 2014 MU69, by the New Horizons spacecraft, colorized with data from earlier images.
Ultima Thule has been called snowman-shaped and peanut-shaped.
(Ultima Thule image from NASA/Johns Hopkins University Applied Physics Laboratory/ Southwest Research Institute, colorized by Renerpho, via Wikimedia Commons.)
The
asteroid,
216 Kleopatra, named after
Egyptian queen,
Cleopatra, was discovered in 1880 by
Austrian astronomer,
Johann Palisa. Kleopatra is much closer to
Earth than Ultima Thule, orbiting in the center of the
asteroid belt between
Mars and
Jupiter at a distance of 2.1-3.5
AU (315-525 million
kilometers). However, because of its small size, just 75
miles (120 kilometers) in extent, it was just just a
point of
light to
terrestrial telescopes.
Radar observations at the turn of the century revealed its peanut shape, although some astronomers prefer to use the equivalent shape designation,
dog-bone. Recent
optical telescope observations have produced more detailed images of this asteroid.[1-3]
Kleopatra has this shape because it's a
contact binary having two elements joined to each other by a
neck of
debris. If its
rotation period of 5.4 hours was much higher, its
lobes would separate to form a
binary system. A huge international team of astronomers used the
European Southern Observatory’s Very Large Telescope (VLT) to capture detailed images of the asteroid Kleopatra. The asteroid was imaged using the
Spectro-Polarimetric High-contrast Exoplanet Research (SPHERE) instrument on the VLT between 2017 and 2019.
Since Kleopatra
rotates, the images were from different
angles, so they allowed creation of an accurate
3D model of its shape. The model showed that one of the lobes is larger than the other, and that the extent of the asteroid is about 270 kilometers. The
density, previously thought to be 4.5
grams per
cubic centimeter, was refined to 3.4.[1,3] Says
Franck Marchis, an astronomer at the
SETI Institute (Mountain View, California) and the
Laboratoire d'Astrophysique de Marseille, France, and leader of the study,
"Kleopatra is truly a unique body in our Solar System... Science makes a lot of progress thanks to the study of weird outliers. I think Kleopatra is one of those and understanding this complex, multiple asteroid system can help us learn more about our Solar System."[3]
Asteroid, 216 Kleopatra from different angles. These images were taken at different times between 2017 and 2019 with the SPHERE instrument on ESO's Very Large Telescope. (ESO/Vernazza, Marchis et al./MISTRAL algorithm (ONERA/CNRS) image, licensed under a Creative Commons Attribution 4.0 International License. Click for larger image.)
Kleopatra has two
moons, named
AlexHelios and
CleoSelene, the names of Cleopatra's children. A companion study used the SPHERE observations to determine the
orbits of these two two moons with better accuracy than previous studies.[2-3] A determination of these orbits was required to correctly determine Kleopatra's
mass, which turned out to be 35% lower than previous
estimates.[3] The mass, along with the
volume, allowed calculation of Kleopatra's density, which is half that of
iron.[3] Since the asteroid is thought to have a
metallic composition, this leads to the conclusion that it's just a
porous pile of
rubble, formed from the remains of a giant
impact.[3]
Since Kleopatra rotates at almost the
speed at which it would start to fling off
material, even small impacts would eject
debris from its surface, and it's thought that its moons, AlexHelios and CleoSelene, were formed in this fashion.[3]
adaptive optics allowed SPHERE to image Kleopatra even though its apparent size on the sky is equivalent to that of a
golf ball at about 40 kilometers distance.[3] ESO has planned a successor to the VLT, appropriately called the
Extremely Large Telescope (ELT).[3]
Size comparison of asteroid, 216 Kleopatra with northern Italy.
Kleopatra is shown as a computer model image.
(ESO/M. Kornmesser/Marchis et al. image, licensed under a Creative Commons Attribution 4.0 International License.)
References:
- F. Marchis, L. Jorda, P. Vernazza, M. Brož, J. Hanuš, M. Ferrais, F. Vachier, N. Rambaux, M. Marsset, M. Viikinkoski, E. Jehin, S. Benseguane, E. Podlewska-Gaca, B. Carry, A. Drouard, S. Fauvaud, M. Birlan, J. Berthier, P. Bartczak, C. Dumas, G. Dudzinski, J. Durech, J. Castillo-Rogez, F. Cipriani, F. Colas, R. Fetick, T. Fusco, J. Grice, A. Kryszczynska, P. Lamy, A. Marciniak, T. Michalowski, P. Michel, M. Pajuelo, T. Santana-Ros, P. Tanga, A. Vigan, O. Witasse and B. Yang, "(216) Kleopatra, a low density critically rotating M-type asteroid," Astronomy & Astrophysics, vol. 653, article no. A57 (September 9, 2021). DOI: 10.1051/0004-6361/202140874. A PDF file can be found at arXiv.
- M. Brož, F. Marchis, L. Jorda, J. Hanuš, P. Vernazza, M. Ferrais, F. Vachier, N. Rambaux, M. Marsset, M. Viikinkoski, E. Jehin, S. Benseguane, E. Podlewska-Gaca, B. Carry, A. Drouard, S. Fauvaud, M. Birlan, J. Berthier, P. Bartczak, C. Dumas, G. Dudzinski, J. Durech, J. Castillo-Rogez, F. Cipriani, F. Colas, R. Fetick, T. Fusco, J. Grice, A. Kryszczynska, P. Lamy, A. Marciniak, T. Michalowski, P. Michel, M. Pajuelo, T. Santana-Ros, P. Tanga, A. Vigan, D. Vokrouhlický, O. Witasse and B. Yang, "An advanced multipole model for (216) Kleopatra triple system," Astronomy & Astrophysics, vol. 653, article no. A56 (September 9, 2021). DOI: 10.1051/0004-6361/202140901. A PDF file can be found at arXiv.
- ESO captures best images yet of peculiar "dog-bone" asteroid, European Southern Observatory Photo Release eso2113, September 9, 2021.
- Location of Kleopatra in the Solar System, European Southern Observatory video, September 9, 2021. Also appears as a YouTube video.