Christopher T. Russell

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Christopher Thomas Russell (born 1943 in St. Albans, England) is head of the Space Physics Center at the Institute of Geophysics and Planetary Physics (IGPP) at UCLA, professor in UCLA's Department of Earth, Planetary, and Space Sciences, and Director of the UCLA Branch of the California Space Grant Consortium. He received a B.Sc. from the University of Toronto in 1964 and a Ph.D. from UCLA in 1968. In 1977 he was awarded the James B. Macelwane Medal [1] and in 2003 the John Adam Fleming Medal [2] by the American Geophysical Union (AGU). He is also a Fellow of the AGU. [3] Asteroid 21459 Chrisrussell was named after him in 2008. [4] In 2017, he was awarded the NASA Distinguished Public Service Medal. [5] He has three grandchildren.

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Research

Selected publications

Related Research Articles

<span class="mw-page-title-main">4 Vesta</span> Second largest asteroid of the main asteroid belt

Vesta is one of the largest objects in the asteroid belt, with a mean diameter of 525 kilometres (326 mi). It was discovered by the German astronomer Heinrich Wilhelm Matthias Olbers on 29 March 1807 and is named after Vesta, the virgin goddess of home and hearth from Roman mythology.

<span class="mw-page-title-main">2 Pallas</span> Third-largest asteroid

Pallas is the second asteroid to have been discovered, after Ceres. It is believed to have a mineral composition similar to carbonaceous chondrite meteorites, like Ceres, though significantly less hydrated than Ceres. It is the third-largest asteroid in the Solar System by both volume and mass, and is a likely remnant protoplanet. It is 79% the mass of Vesta and 22% the mass of Ceres, constituting an estimated 7% of the mass of the asteroid belt. Its estimated volume is equivalent to a sphere 507 to 515 kilometers in diameter, 90–95% the volume of Vesta.

<i>Dawn</i> (spacecraft) NASA mission to study main-belt asteroids via a robotic probe (2007–18)

Dawn is a retired space probe that was launched by NASA in September 2007 with the mission of studying two of the three known protoplanets of the asteroid belt: Vesta and Ceres. In the fulfillment of that mission—the ninth in NASA's Discovery Program—Dawn entered orbit around Vesta on July 16, 2011, and completed a 14-month survey mission before leaving for Ceres in late 2012. It entered orbit around Ceres on March 6, 2015. In 2017, NASA announced that the planned nine-year mission would be extended until the probe's hydrazine fuel supply was depleted. On November 1, 2018, NASA announced that Dawn had depleted its hydrazine, and the mission was ended. The derelict probe remains in a stable orbit around Ceres.

<span class="mw-page-title-main">704 Interamnia</span> Large asteroid in the asteroid belt

704 Interamnia is a large F-type asteroid. With a mean diameter of around 330 kilometres, it is the fifth-largest asteroid, after Ceres, Vesta, Pallas and Hygiea. Its mean distance from the Sun is 3.067 AU. It was discovered on 2 October 1910 by Vincenzo Cerulli, and named after the Latin name for Teramo, Italy, where Cerulli worked. Its mass is probably between fifth and tenth highest in the asteroid belt, with a mass estimated to be 1.2% of the mass of the entire asteroid belt. Observations by the Very Large Telescope's SPHERE imager in 2017–2019, combined with occultation results, indicate that the shape of Interamnia may be consistent with hydrostatic equilibrium for a body of its density with a rotational period of 7.6 hours. This suggests that Interamnia may have formed as an equilibrium body, and that impacts changed its rotational period after it fully solidified.

<span class="mw-page-title-main">Ceres (dwarf planet)</span> Dwarf planet in the asteroid belt

Ceres, minor-planet designation 1 Ceres, is a dwarf planet in the middle main asteroid belt between the orbits of Mars and Jupiter. It was the first asteroid discovered on 1 January 1801, by Giuseppe Piazzi at Palermo Astronomical Observatory in Sicily and announced as a new planet. Ceres was later classified as an asteroid and then a dwarf planet, the only one always inside Neptune's orbit.

<span class="mw-page-title-main">GRAIL</span> 2011–12 NASA mission to study the Moons geology

The Gravity Recovery and Interior Laboratory (GRAIL) was an American lunar science mission in NASA's Discovery Program which used high-quality gravitational field mapping of the Moon to determine its interior structure. The two small spacecraft GRAIL A (Ebb) and GRAIL B (Flow) were launched on 10 September 2011 aboard a single launch vehicle: the most-powerful configuration of a Delta II, the 7920H-10. GRAIL A separated from the rocket about nine minutes after launch, GRAIL B followed about eight minutes later. They arrived at their orbits around the Moon 25 hours apart. The first probe entered orbit on 31 December 2011 and the second followed on 1 January 2012. The two spacecraft impacted the Lunar surface on December 17, 2012.

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<span class="mw-page-title-main">Rheasilvia</span> Impact crater on the surface of the asteroid 4 Vesta

Rheasilvia is the most prominent surface feature on the asteroid Vesta and is thought to be an impact crater. It is 505 km (314 mi) in diameter, which is 90% the diameter of Vesta itself, and is 95% the mean diameter of Vesta, 529 km (329 mi). However, the mean is affected by the crater itself. It is 89% the mean equatorial diameter of 569 km (354 mi), making it one of the largest craters in the Solar System, and at 75°S latitude, covers most of the southern hemisphere. The peak in the center of the crater is 200 km (120 mi) in diameter, and rises 22.5 km from its base, making it one of the tallest mountains known in the Solar System.

<span class="mw-page-title-main">David Southwood</span>

David John Southwood is a British space scientist who holds the post of Senior Research Investigator at Imperial College London. He was the President of the Royal Astronomical Society from 2012–2014, and earlier served as the Director of Science and Robotic Exploration at the European Space Agency (2001–2011). Southwood's research interests have been in solar–terrestrial physics and planetary science, particularly magnetospheres. He built the magnetic field instrument for the Cassini Saturn orbiter.

<span class="mw-page-title-main">Margaret G. Kivelson</span> American geophysicist, planetary scientist (born 1928)

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<span class="mw-page-title-main">Alexander J. Dessler</span> American astrophysicist (1928–2023)

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References

  1. "James B. Macelwane Medal". American Geophysical Union. Archived from the original on June 6, 2011. Retrieved March 17, 2011.
  2. "Christopher T. Russell receives 2003 John Adam Fleming Medal". American Geophysical Union. Retrieved March 17, 2003.[ permanent dead link ]
  3. "Russell - AGU Honors Program".
  4. Minor Planet Circulars, International Astronomical Union: 63393, 2008-07-13{{citation}}: Missing or empty |title= (help)
  5. "NASA's 2017 Distinguished Public Service Medal Honorees". NASA.
  6. "NASA's Polar Mission: Unlocking the Secrets of Earth's Magnetosphere". National Aeronautics and Space Administration. Retrieved March 17, 2011.
  7. "Dawn mission gets Vesta asteroid target practice", Science Daily, March 13, 2011, retrieved March 17, 2011.