Shantanu Basu | |
---|---|
Born | October 5, 1964 |
Nationality | American |
Alma mater | University of Illinois at Urbana-Champaign |
Known for | Migrating Embryo Model for Protoplanetary Disk Evolution |
Scientific career | |
Fields | Star Formation |
Institutions | |
Website | shantanubasu |
Shantanu Basu (born October 5, 1964) is an American astrophysicist and Professor in the Department of Physics and Astronomy at the Canadian University of Western Ontario, in London, Ontario. [1] [2] . Beginning in 2025, he will serve as interim director at the Canadian Institute for Theoretical Astrophysics, located at the University of Toronto. [3]
Basu received his PhD in Physics from the University of Illinois at Urbana-Champaign in 1993, and held academic positions at Michigan State University and the Canadian Institute for Theoretical Astrophysics, in Toronto, before joining Western in 1999. Basu has made contributions to understanding the fragmentation of interstellar molecular clouds, the role of magnetic fields and angular momentum in gravitational collapse and star formation, the origin of luminosity bursts from young stellar objects, and the origin of power-laws in the mass distribution of stars. He is one of the originators of the Migrating Embryo Model for protoplanetary disk evolution, which is a unified scenario for angular momentum transport, binary star and giant planet formation, and the formation of ejected freely floating low mass objects. [4]
Asteroid 277883 Basu, discovered by Canadian astronomer Paul Wiegert at the Mauna Kea Observatories in 2006, was named in his honor. The official naming citation was published by the Minor Planet Center on September 19, 2013 ( M.P.C. 85018). [5] [6]
The following outline is provided as an overview and topical guide to space science:
Planetesimals are solid objects thought to exist in protoplanetary disks and debris disks. Believed to have formed in the Solar System about 4.6 billion years ago, they aid study of its formation.
The nebular hypothesis is the most widely accepted model in the field of cosmogony to explain the formation and evolution of the Solar System. It suggests the Solar System is formed from gas and dust orbiting the Sun which clumped up together to form the planets. The theory was developed by Immanuel Kant and published in his Universal Natural History and Theory of the Heavens (1755) and then modified in 1796 by Pierre Laplace. Originally applied to the Solar System, the process of planetary system formation is now thought to be at work throughout the universe. The widely accepted modern variant of the nebular theory is the solar nebular disk model (SNDM) or solar nebular model. It offered explanations for a variety of properties of the Solar System, including the nearly circular and coplanar orbits of the planets, and their motion in the same direction as the Sun's rotation. Some elements of the original nebular theory are echoed in modern theories of planetary formation, but most elements have been superseded.
A protostar is a very young star that is still gathering mass from its parent molecular cloud. It is the earliest phase in the process of stellar evolution. For a low-mass star, it lasts about 500,000 years. The phase begins when a molecular cloud fragment first collapses under the force of self-gravity and an opaque, pressure-supported core forms inside the collapsing fragment. It ends when the infalling gas is depleted, leaving a pre-main-sequence star, which contracts to later become a main-sequence star at the onset of hydrogen fusion producing helium.
A protoplanetary disk is a rotating circumstellar disc of dense gas and dust surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star. The protoplanetary disk may not be considered an accretion disk, while the two are similar. While they are similar, an accretion disk is hotter, and spins much faster. It is also found on black holes, not stars. This process should not be confused with the accretion process thought to build up the planets themselves. Externally illuminated photo-evaporating protoplanetary disks are called proplyds.
David Clifford Jewitt is a British-American astronomer who studies the Solar System, especially its minor bodies. He is based at the University of California, Los Angeles, where he is a Member of the Institute for Geophysics and Planetary Physics, the Director of the Institute for Planets and Exoplanets, Professor of Astronomy in the Department of Physics and Astronomy and Professor of Astronomy in the Department of Earth, Planetary and Space Sciences. He is best known for being the first person to discover a body beyond Pluto and Charon in the Kuiper belt.
Planetary migration occurs when a planet or other body in orbit around a star interacts with a disk of gas or planetesimals, resulting in the alteration of its orbital parameters, especially its semi-major axis. Planetary migration is the most likely explanation for hot Jupiters. The generally accepted theory of planet formation from a protoplanetary disk predicts that such planets cannot form so close to their stars, as there is insufficient mass at such small radii and the temperature is too high to allow the formation of rocky or icy planetesimals.
In astrophysics, accretion is the accumulation of particles into a massive object by gravitationally attracting more matter, typically gaseous matter, into an accretion disk. Most astronomical objects, such as galaxies, stars, and planets, are formed by accretion processes.
The following outline is provided as an overview of and topical guide to astronomy:
(612911) 2004 XR190, informally nicknamed Buffy, is a trans-Neptunian object, classified as both a scattered disc object and a detached object, located in the outermost region of the Solar System. It was first observed on 11 December 2004, by astronomers with the Canada–France Ecliptic Plane Survey at the Mauna Kea Observatories, Hawaii, United States. It is the largest known highly inclined (> 45°) object. With a perihelion of 51 AU, it belongs to a small and poorly understood group of very distant objects with moderate eccentricities.
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.
Julianne Dalcanton is an American astronomer, professor of astronomy, researcher and comet discoverer. Since September 2021 she is the director of the Simons Foundation Center for Computational Astrophysics.
Grove Creek Observatory is an astronomical observatory in Trunkey Creek, New South Wales, Australia. The site also hosts remote-controlled telescopes in three separate enclosings. It is located about four hours' drive from Sydney, Australia. It is run by Jim Lynch and Greg Ford.
Retrograde motion in astronomy is, in general, orbital or rotational motion of an object in the direction opposite the rotation of its primary, that is, the central object. It may also describe other motions such as precession or nutation of an object's rotational axis. Prograde or direct motion is more normal motion in the same direction as the primary rotates. However, "retrograde" and "prograde" can also refer to an object other than the primary if so described. The direction of rotation is determined by an inertial frame of reference, such as distant fixed stars.
In planetary astronomy, the grand tack hypothesis proposes that Jupiter formed at a distance of 3.5 AU from the Sun, then migrated inward to 1.5 AU, before reversing course due to capturing Saturn in an orbital resonance, eventually halting near its current orbit at 5.2 AU. The reversal of Jupiter's planetary migration is likened to the path of a sailboat changing directions (tacking) as it travels against the wind.
A circumstellar disc is a torus, pancake or ring-shaped accretion disk of matter composed of gas, dust, planetesimals, asteroids, or collision fragments in orbit around a star. Around the youngest stars, they are the reservoirs of material out of which planets may form. Around mature stars, they indicate that planetesimal formation has taken place, and around white dwarfs, they indicate that planetary material survived the whole of stellar evolution. Such a disc can manifest itself in various ways.
Nicholas Kaiser was a British cosmologist. He is the son of Thomas Reeve Kaiser.
(523635) 2010 DN93 (provisional designation 2010 DN93) is a trans-Neptunian object from in the scattered disc located in the outermost region of the Solar System. It was discovered on 26 February 2010, by astronomers with the Pan-STARRS survey at Haleakala Observatory on the island of Maui, Hawaii, in the United States. Assuming a low albedo, the object is estimated at approximately 490 kilometers (300 miles) in diameter. It was numbered in 2018 and remains unnamed.
Sergei Ivanovich Ipatov is a Soviet, Russian, and American scientist, laureate of the F. A. Bredikhin Prize in astronomy of the Russian Academy of Sciences, Doctor of Physical and Mathematical Sciences. Asteroid 14360 Ipatov was named in his honor.