Robin Canup

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Robin M. Canup (born November 20, 1968) is an American astrophysicist. Her main area of research concerns the origins of planets and satellites. [1] In 2003, Canup was awarded the Harold C. Urey Prize. [2] In April, 2022, Canup presented the findings of the Planetary Science Decadal Survey as co-chair of the Survey Steering Committee with Philip R. Christensen. [3]

Contents

Biography

She received her B.S. from Duke University and her PhD from the University of Colorado at Boulder.

Canup is known for her research based upon the giant impact hypothesis, using intensive modeling to simulate how planetary collisions unfold. [4] [5] [6] [7] In 2012, Canup first published a refinement to the giant impact hypothesis, arguing that the Moon and the Earth formed in a series of steps that started with a massive collision of two planetary bodies, each larger than Mars, which then re-collided to form what we now call Earth. [8] After the re-collision, Earth was surrounded by a disk of material, which combined to form the Moon. [9] She has written a book on the origin of the Earth and Moon. [10] Canup has also published research describing a giant impact origin for Pluto and Charon. [11]

Canup is an accomplished ballet dancer and danced the lead role in Coppélia in the Boulder Ballet one week after finishing her dissertation. [12]

Selected works

Related Research Articles

<span class="mw-page-title-main">Moon</span> Natural satellite orbiting Earth

The Moon is Earth's only natural satellite. It orbits at an average distance of 384,400 km (238,900 mi), about 30 times Earth's diameter. The Moon always presents the same side to Earth, because gravitational pull has locked its rotation to the planet. This results in the lunar day of 29.5 Earth days matching the lunar month. The Moon's gravitational pull – and to a lesser extent the Sun's – are the main drivers of the tides.

<span class="mw-page-title-main">Callisto (moon)</span> Second-largest moon of Jupiter

Callisto, or Jupiter IV, is the second-largest moon of Jupiter, after Ganymede. In the Solar System it is the third-largest moon after Ganymede and Saturn's largest moon Titan, and as large as the smallest planet Mercury, though only about a third as massive. Callisto is, with a diameter of 4,821 km, roughly a third larger than Earth's Moon and orbits Jupiter on average at a distance of 1,883,000 km, which is about six times further out than the Moon orbiting Earth. It is the outermost of the four large Galilean moons of Jupiter, which were discovered in 1610 with one of the first telescopes, being visible from Earth with common binoculars.

<span class="mw-page-title-main">Giant-impact hypothesis</span> Theory of the formation of the Moon

The giant-impact hypothesis, sometimes called the Big Splash, or the Theia Impact, is an astrogeology hypothesis for the formation of the Moon first proposed in 1946 by Canadian geologist Reginald Daly. The hypothesis suggests that the Early Earth collided with a Mars-sized dwarf planet of the same orbit approximately 4.5 billion years ago in the early Hadean eon, and the ejectae of the impact event later accreted to form the Moon. The impactor planet is sometimes called Theia, named after the mythical Greek Titan who was the mother of Selene, the goddess of the Moon.

<span class="mw-page-title-main">Charon (moon)</span> Largest natural satellite of Pluto

Charon, known as (134340) Pluto I, is the largest of the five known natural satellites of the dwarf planet Pluto. It has a mean radius of 606 km (377 mi). Charon is the sixth-largest known trans-Neptunian object after Pluto, Eris, Haumea, Makemake and Gonggong. It was discovered in 1978 at the United States Naval Observatory in Washington, D.C., using photographic plates taken at the United States Naval Observatory Flagstaff Station (NOFS).

<span class="mw-page-title-main">Phobos (moon)</span> Largest and innermost moon of Mars

Phobos is the innermost and larger of the two natural satellites of Mars, the other being Deimos. The two moons were discovered in 1877 by American astronomer Asaph Hall. It is named after Phobos, the Greek god of fear and panic, who is the son of Ares (Mars) and twin brother of Deimos.

<span class="mw-page-title-main">Natural satellite</span> Astronomical body that orbits a planet

A natural satellite is, in the most common usage, an astronomical body that orbits a planet, dwarf planet, or small Solar System body. Natural satellites are colloquially referred to as moons, a derivation from the Moon of Earth.

<span class="mw-page-title-main">Impact event</span> Collision of two astronomical objects

An impact event is a collision between astronomical objects causing measurable effects. Impact events have physical consequences and have been found to regularly occur in planetary systems, though the most frequent involve asteroids, comets or meteoroids and have minimal effect. When large objects impact terrestrial planets such as the Earth, there can be significant physical and biospheric consequences, though atmospheres mitigate many surface impacts through atmospheric entry. Impact craters and structures are dominant landforms on many of the Solar System's solid objects and present the strongest empirical evidence for their frequency and scale.

<span class="mw-page-title-main">Tholin</span> Class of molecules formed by ultraviolet irradiation of organic compounds

Tholins are a wide variety of organic compounds formed by solar ultraviolet or cosmic ray irradiation of simple carbon-containing compounds such as carbon dioxide, methane or ethane, often in combination with nitrogen or water. Tholins are disordered polymer-like materials made of repeating chains of linked subunits and complex combinations of functional groups, typically nitriles and hydrocarbons, and their degraded forms such as amines and phenyls. Tholins do not form naturally on modern-day Earth, but they are found in great abundance on the surfaces of icy bodies in the outer Solar System, and as reddish aerosols in the atmospheres of outer Solar System planets and moons.

<span class="mw-page-title-main">Erik Ian Asphaug</span> American astronomer

Erik Ian Asphaug is a Norwegian American planetary science professor in the School of Earth and Space Exploration at University of Arizona. Asphaug received his bachelor's degree in mathematics and English from Rice University and his PhD in planetary science from the University of Arizona.

<span class="mw-page-title-main">Nix (moon)</span> Moon of Pluto

Nix is a natural satellite of Pluto, with a diameter of 49.8 km (30.9 mi) across its longest dimension. It was discovered along with Pluto's outermost moon Hydra on 15 May 2005 by astronomers using the Hubble Space Telescope, and was named after Nyx, the Greek goddess of the night. Nix is the third moon of Pluto by distance, orbiting between the moons Styx and Kerberos.

<span class="mw-page-title-main">Hydra (moon)</span> Moon of Pluto

Hydra is a natural satellite of Pluto, with a diameter of approximately 51 km (32 mi) across its longest dimension. It is the second-largest moon of Pluto, being slightly larger than Nix. Hydra was discovered along with Nix by astronomers using the Hubble Space Telescope on 15 May 2005, and was named after the Hydra, the nine-headed underworld serpent in Greek mythology. By distance, Hydra is the fifth and outermost moon of Pluto, orbiting beyond Pluto's fourth moon Kerberos.

<span class="mw-page-title-main">Moons of Pluto</span> Natural satellites orbiting Pluto

The dwarf planet Pluto has five natural satellites. In order of distance from Pluto, they are Charon, Styx, Nix, Kerberos, and Hydra. Charon, the largest, is mutually tidally locked with Pluto, and is massive enough that Pluto–Charon is sometimes considered a double dwarf planet.

<span class="mw-page-title-main">Formation and evolution of the Solar System</span> Modelling its structure and composition

There is evidence that the formation of the Solar System began about 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.

<span class="mw-page-title-main">Lunar magma ocean</span> Theorized historical geological layer on the Moon

The Lunar Magma Ocean (LMO) is the layer of molten rock that is theorized to have been present on the surface of the Moon. The Lunar Magma Ocean was likely present on the Moon from the time of the Moon's formation to tens or hundreds of millions of years after that time. It is a thermodynamic consequence of the Moon's relatively rapid formation in the aftermath of a giant impact between the proto-Earth and another planetary body. As the Moon accreted from the debris from the giant impact, gravitational potential energy was converted to thermal energy. Due to the rapid accretion of the Moon, thermal energy was trapped since it did not have sufficient time to thermally radiate away energy through the lunar surface. The subsequent thermochemical evolution of the Lunar Magma Ocean explains the Moon's largely anorthositic crust, europium anomaly, and KREEP material.

<span class="mw-page-title-main">Regular moon</span> Satellites which formed around their parent planet

In astronomy, a regular moon or a regular satellite is a natural satellite following a relatively close, stable, and circular orbit which is generally aligned to its primary's equator. They formed within of discs of debris which surround their primary, usually the aftermath of a large collision or material accumulated from the protoplanetary disc. These debris discs then accrete into regular moons, as opposed to irregular moons, which were captured.

<span class="mw-page-title-main">Late Heavy Bombardment</span> Hypothesized astronomical event

The Late Heavy Bombardment (LHB), or lunar cataclysm, is a hypothesized astronomical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, at a time corresponding to the Neohadean and Eoarchean eras on Earth. According to the hypothesis, during this interval, a disproportionately large number of asteroids and comets collided into the terrestrial planets and their natural satellites of the inner Solar System, including Mercury, Venus, Earth and Mars. These came from both post-accretion and planetary instability-driven populations of impactors. Although it used to be widely accepted, it remained difficult to provide an overwhelming amount of evidence for the hypothesis. However, recent re-appraisal of the cosmo-chemical constraints indicates that there was likely no late spike in the bombardment rate.

<span class="mw-page-title-main">Origin of the Moon</span> Theories explaining the formation of Earths Moon

The origin of the Moon is usually explained by a Mars-sized body striking the Earth, creating a debris ring that eventually collected into a single natural satellite, the Moon, but there are a number of variations on this giant-impact hypothesis, as well as alternative explanations, and research continues into how the Moon came to be formed. Other proposed scenarios include captured body, fission, formed together, planetesimal collisions, and collision theories.

<span class="mw-page-title-main">Theia (planet)</span> Planet hypothesized to have impacted Earth and created the Moon

Theia is a hypothesized ancient planet in the early Solar System that, according to the giant-impact hypothesis, collided with the early Earth around 4.5 billion years ago, with some of the resulting ejected debris gathering to form the Moon. Such a collision, with the two planets' cores and mantles fusing, could explain why Earth's core is larger than expected for a body its size. Collision simulations support the idea that the large low-shear-velocity provinces in the lower mantle may be remnants of Theia. Theia is hypothesized to have been about the size of Mars, and may have formed in the outer Solar System and provided much of Earth's water.

<span class="mw-page-title-main">Satellite system (astronomy)</span> Set of gravitationally bound objects in orbit

A satellite system is a set of gravitationally bound objects in orbit around a planetary mass object or minor planet, or its barycenter. Generally speaking, it is a set of natural satellites (moons), although such systems may also consist of bodies such as circumplanetary disks, ring systems, moonlets, minor-planet moons and artificial satellites any of which may themselves have satellite systems of their own. Some bodies also possess quasi-satellites that have orbits gravitationally influenced by their primary, but are generally not considered to be part of a satellite system. Satellite systems can have complex interactions including magnetic, tidal, atmospheric and orbital interactions such as orbital resonances and libration. Individually major satellite objects are designated in Roman numerals. Satellite systems are referred to either by the possessive adjectives of their primary, or less commonly by the name of their primary. Where only one satellite is known, or it is a binary with a common centre of gravity, it may be referred to using the hyphenated names of the primary and major satellite.

<span class="mw-page-title-main">Dimorphos</span> Moon of asteroid Didymos

Dimorphos is a natural satellite or moon of the near-Earth asteroid 65803 Didymos, with which it forms a binary system. The moon was discovered on 20 November 2003 by Petr Pravec in collaboration with other astronomers worldwide. Dimorphos has a diameter of 177 meters (581 ft) across its longest extent and it was the target of the Double Asteroid Redirection Test (DART), a NASA space mission that deliberately collided a spacecraft with the moon on 26 September 2022 to alter its orbit around Didymos. Before the impact by DART, Dimorphos had a shape of an oblate spheroid with a surface covered in boulders but virtually no craters. The moon is thought to have formed when Didymos shed its mass due to its rapid rotation, which formed an orbiting ring of debris that conglomerated into a low-density rubble pile that became Dimorphos today.

References

  1. University of Boulder Profile, boulder.swri.edu; accessed March 9, 2015.
  2. "Harold C. Urey Prize in Planetary Science". Division of Planetary Sciences of the American Astronomical Association. Retrieved 2015-01-12.
  3. "Planetary Science and Astrobiology Decadal Survey 2023 2032 | National Academies".
  4. Canup, Robin M.; Asphaug, Erik (2001-08-16). "Origin of the Moon in a giant impact near the end of the Earth's formation". Nature. 412 (6848): 708–712. Bibcode:2001Natur.412..708C. doi:10.1038/35089010. ISSN   0028-0836. PMID   11507633. S2CID   4413525.
  5. Agnor, Craig B.; Canup, Robin M.; Levison, Harold F. (1999). "On the Character and Consequences of Large Impacts in the Late Stage of Terrestrial Planet Formation". Icarus. 142 (1): 219–237. Bibcode:1999Icar..142..219A. doi:10.1006/icar.1999.6201. ISSN   0019-1035. S2CID   28238627.
  6. Canup, Robin M. (2004). "Simulations of a late lunar-forming impact". Icarus. 168 (2): 433–456. Bibcode:2004Icar..168..433C. doi:10.1016/j.icarus.2003.09.028. ISSN   0019-1035.
  7. Canup, Robin M. (2004). "Dynamics of Lunar Formation". Annual Review of Astronomy and Astrophysics. 42 (1): 441–475. Bibcode:2004ARA&A..42..441C. doi:10.1146/annurev.astro.41.082201.113457.
  8. Canup, Robin M. (2012-11-23). "Forming a Moon with an Earth-like Composition via a Giant Impact". Science . 338 (6110): 1052–1055. Bibcode:2012Sci...338.1052C. doi:10.1126/science.1226073. PMC   6476314 . PMID   23076098.
  9. "NASA Lunar Scientists Develop New Theory on Earth and Moon Formation". NASA Press Release. NASA. 2012-10-30. Archived from the original on 2019-02-23. Retrieved 2012-12-05.
  10. Origin of the Earth and Moon. Robin M. Canup, Kevin Righter (eds.) (2nd ed.). Tucson : Houston: University of Arizona Press. 2000-11-01. ISBN   978-0-8165-2073-2.{{cite book}}: CS1 maint: others (link)
  11. Canup, Robin M. (2005-01-28). "A Giant Impact Origin of Pluto-Charon". Science. 307 (5709): 546–550. Bibcode:2005Sci...307..546C. doi:10.1126/science.1106818. ISSN   1095-9203. PMID   15681378. S2CID   19558835.
  12. Finn, Ed (2004-10-29). "Robin Canup". Popular Science . Retrieved 2015-10-13.