Steven Soter

Last updated
Steven Soter
Alma mater University of California, Los Angeles (Astronomy & physics)
Cornell University (Ph.D)
Known for Cosmos: A Personal Voyage , Cosmos: A Spacetime Odyssey
Awards Primetime Emmy Award (for writing of Cosmos)
Scientific career
Fields Physical cosmology, astrophysics
Doctoral advisors Thomas Gold, Carl Sagan, Joseph Burns

Steven Soter is an astrophysicist currently holding the positions of scientist-in-residence for New York University's Environmental Studies Program and of Research Associate for the Department of Astrophysics at the American Museum of Natural History. He is a proponent of the International Astronomical Union's definition of planet.

Contents

Education

Soter received his bachelor's degree in astronomy and physics from UCLA in 1965 (advisors George Abell and Peter Goldreich) and his doctorate in astronomy from Cornell University in 1971 (advisors Thomas Gold, Carl Sagan, and Joseph Burns).

Career in astrophysics

In 1974, Soter suggested that dust produced by meteoritic bombardment of Saturn's moon Phoebe might orbit the planet until colliding with Saturn's moon Iapetus and be responsible for the unique dark-bright dichotomy of the latter. Although not the unique cause, dust originating from Saturn's irregular satellites was later found in data from the Cassini spacecraft to indeed play a crucial role in the coloration of Iapetus. [1] [2] The discovery of Saturn's "Phoebe ring" in 2009 further strengthened the probability that this process first described by Soter plays a significant role in shaping Iapetus's appearance. [3] [4]

In 1977-1979, Soter co-wrote, along with Carl Sagan and Ann Druyan, Carl Sagan's monumental 1980 astronomy documentary series Cosmos . Since then, he has also acted as advisor on a number of science documentaries, such as the IMAX films Blue Planet and Cosmic Voyage .

In 1997, Soter took a position at the American Museum of Natural History's Hayden Planetarium, and eventually progressed to the position of research associate. He also made significant contributions to research related to the ancient Greek city Helike.

In 2007, after the IAU voted on a definition of planet, Soter published an article [5] in Scientific American in which he outlined a mathematical formulation, the "planetary discriminant," to describe how the IAU's requirement that a planet must have "cleared its neighborhood" of other objects might be applied in practice. He had already written a more technical article on the same subject in 2006, submitted to The Astronomical Journal before the IAU resolution. [6]

In 2014, he partnered with Druyan again to co-write a new television miniseries, Cosmos: A Spacetime Odyssey , hosted by his AMNH colleague Neil deGrasse Tyson.

Related Research Articles

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<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">Rhea (moon)</span> Moon of Saturn

Rhea is the second-largest moon of Saturn and the ninth-largest moon in the Solar System, with a surface area that is comparable to the area of Australia. It is the smallest body in the Solar System for which precise measurements have confirmed a shape consistent with hydrostatic equilibrium. It was discovered in 1672 by Giovanni Domenico Cassini.

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

Tethys, or Saturn III, is a mid-sized moon of Saturn about 1,060 km (660 mi) across. It was discovered by G. D. Cassini in 1684 and is named after the titan Tethys of Greek mythology.

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

Iapetus is a moon of Saturn. With an estimated diameter of 1,469 km, it is the third-largest moon of Saturn and the eleventh-largest in the Solar System. Named after the Titan Iapetus, the moon was discovered in 1671 by Giovanni Domenico Cassini.

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

Hyperion, also known as Saturn VII, is a moon of Saturn discovered by William Cranch Bond, his son George Phillips Bond and William Lassell in 1848. It is distinguished by its irregular shape, its chaotic rotation, and its unexplained sponge-like appearance. It was the first non-round moon to be discovered.

<span class="mw-page-title-main">Himalia (moon)</span> Moon of Jupiter (Jupiter VI)

Himalia, or Jupiter VI, is the largest irregular satellite of Jupiter, with a diameter of at least 140 km (90 mi). It is the sixth largest Jovian satellite, after the four Galilean moons and Amalthea. It was discovered by Charles Dillon Perrine at the Lick Observatory on 3 December 1904 and is named after the nymph Himalia, who bore three sons of Zeus. It is one of the largest planetary moons in the Solar System not imaged in detail, and the third largest not imaged in detail within the orbit of Neptune.

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

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<span class="mw-page-title-main">Moons of Saturn</span> Natural satellites of the planet Saturn

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Siarnaq, also designated Saturn XXIX, is the second-largest irregular moon of Saturn. It was discovered on 23 September 2000 by a team of astronomers led by Brett J. Gladman. It was named after the Inuit goddess of the sea, Siarnaq, who is more commonly known as Sedna. Siarnaq is the largest member of Saturn's Inuit group of prograde irregular moons, which orbit far from Saturn in the same direction as the planet's rotation. The moons of the Inuit group are believed to have originated as fragments from the collisional breakup of a larger progenitor moon after it was gravitationally captured into orbit around Saturn several billion years ago. Several other small Inuit group moons share similar orbits to Siarnaq, indicating that the moon had experienced another collision after forming from its progenitor.

The definition of the term planet has changed several times since the word was coined by the ancient Greeks. Greek astronomers employed the term ἀστέρες πλανῆται, 'wandering stars', for star-like objects which apparently moved over the sky. Over the millennia, the term has included a variety of different celestial bodies, from the Sun and the Moon to satellites and asteroids.

<span class="mw-page-title-main">Rings of Saturn</span> Planar assemblage of icy particles orbiting Saturn

The rings of Saturn are the most extensive ring system of any planet in the Solar System. They consist of countless small particles, ranging in size from micrometers to meters, that orbit around Saturn. The ring particles are made almost entirely of water ice, with a trace component of rocky material. There is still no consensus as to their mechanism of formation. Although theoretical models indicated that the rings were likely to have formed early in the Solar System's history, newer data from Cassini suggested they formed relatively late.

<span class="mw-page-title-main">Carolyn Porco</span> American planetary scientist

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<span class="mw-page-title-main">Planetary-mass moon</span> Planetary-mass bodies that are also natural satellites

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<span class="mw-page-title-main">Subsatellite</span> A satellite that orbits a natural satellite

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<span class="mw-page-title-main">Equatorial ridge on Iapetus</span> Terrain feature on Saturns third-largest moon

The equatorial ridge is the tallest mountain feature on Saturn's moon Iapetus. It is 20 km (12 mi) high, and is the third tallest mountain structure in the Solar System. It runs along most of Iapetus' equator. It was discovered by the Cassini probe in 2004. The ridge's origin is unknown. There are bright areas on the sides of the equatorial ridge near Iapetus' bright trailing hemisphere, which were already visible in Voyager 2 images appearing like mountains and were nicknamed the "Voyager Mountains".

The International Union of Geological Sciences (IUGS) is the internationally recognized body charged with fostering agreement on nomenclature and classification across geoscientific disciplines. However, they have yet to create a formal definition of the term planet. As a result, there are various geophysical definitions in use among professional geophysicists, planetary scientists, and other professionals in the geosciences. Many professionals opt to use one of several of these geophysical definitions instead of the definition voted on by the International Astronomical Union.

References

  1. Denk, Tilmann; Neukum, Gerhard; Roatsch, Thomas; Porco, Carolyn C.; Burns, Joseph A.; Galuba, Götz G.; Schmedemann, Nico; Helfenstein, Paul; Thomas, Peter C. (2010-01-22). "Iapetus: Unique Surface Properties and a Global Color Dichotomy from Cassini Imaging". Science . 327 (5964): 435–439. Bibcode:2010Sci...327..435D. doi:10.1126/science.1177088. PMID   20007863. S2CID   165865.
  2. Spencer, John R.; Denk, Tilmann (2010-01-22). "Formation of Iapetus' Extreme Albedo Dichotomy by Exogenically Triggered Thermal Ice Migration". Science . 327 (5964): 432–435. Bibcode:2010Sci...327..432S. CiteSeerX   10.1.1.651.4218 . doi:10.1126/science.1177132. PMID   20007862. S2CID   20663944.
  3. Verbiscer, Anne; Skrutskie, Michael; Hamilton, Douglas (2009-10-07). "Saturn's largest ring". Nature . 461 (7267): 1098–100. Bibcode:2009Natur.461.1098V. doi:10.1038/nature08515. PMID   19812546. S2CID   4349726.
  4. Cowen, Rob (2009-10-06). "Largest known planetary ring discovered". Science News .
  5. Soter, Steven (2007). "What Is a Planet?" (PDF). Scientific American. 296 (1): 34–41. arXiv: astro-ph/0608359 . Bibcode:2007SciAm.296a..34S. doi:10.1038/scientificamerican0107-34. PMID   17186831.
  6. Soter, Steven (2006). "What Is a Planet?". The Astronomical Journal. 132 (6): 2513–2519. arXiv: astro-ph/0608359 . Bibcode:2006AJ....132.2513S. doi:10.1086/508861. ISSN   0004-6256. S2CID   14676169.