Медаль Джеймса Крейга Уотсона (англ.James Craig Watson Medal) — награда, присуждаемая раз в два года Национальной академией наук США за вклад в астрономию. Названа в честь канадско-американского астронома Д. К. Уотсона, на средства которого учреждена. Вместе с бронзовой медалью лауреату вручаются $25 000 и $50 000 направляются на поддержку его исследований[1].
Награждённые медалью Джеймса Крейга Уотсона
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For his work in perfecting the application of heliometer to astronomical measurements, which has resulted in an important advance in astronomy of precision, especially in the determination of parallaxes of the sun and stars and of the position of the planets.
For the skill and ability shown in supervising the preparation of the tables of the Watson asteroids, involving original methods, and leading to results of value to celestial mechanics.
For his observations of solar eclipses, in particular a detailed study of the spectrum of the chromosphere which has contributed notably to our knowledge of the sun's atmosphere.
For his scientific accomplishments in celestial mechanics and orbit computation, and particularly for his contributions to the knowledge of the orbits of asteroids.
In recognition of his resolution of the problem of lunar motion around the earth through his adaption of modern computing machinery to algebraic rather than arithmetic operations.
For his long and distinguished career in Dynamical Astronomy and his independent determination of a completely new and more accurate Theory of the Motion of Mars.
For his contributions to the dynamics of solar-system bodies, especially for calculations leading to the prediction of volcanic action on Io, dramatically verified by Voyager photography.
For his work in the area of image enhancement and galactic dynamics, which has contributed greatly to the characterization of the unseen matter in galaxies.
For his work as creator and exploiter of new instruments and techniques that have opened whole new areas of astronomy to us all--solar oscillations, infrared surveys, spun telescopes, and large millimeter-wave reflectors.
First to grasp the extraordinary distances and luminosities of quasi-stellar sources and a pioneer in their use to probe the outer limits of our universe.
For his leadership in X-ray astronomy since its beginning, and his crucial role in enabling the U.S./Japanese collaboration in the ASCA mission, a beautiful example of international cooperation in sciences.
For their painstaking research, which led to the discovery of more than 800 asteroids and 32 comets, including their co-discovery of Comet Shoemaker-Levy, the first comet observed colliding with a planet.
For elegant precision measurements by Wilkinson, his students, and their students, of universal radiation that is close to blackbody yet wonderfully rich in evidence of cosmic evolution.
For her seminal observations of dark matter in galaxies, large-scale relative motions of galaxies, and for generous mentoring of young astronomers, men and women.
For their monumental work in developing and completing the Two Micron All-Sky Survey, thus enabling a thrilling variety of explorations in astronomy and astrophysics.
For her role in critical discoveries concerning the large-scale structure of the Universe, for her insightful analyses of galaxies in groups and clusters, and for her being a model in mentoring young scientists.
For his seminal contributions to the theory of the interstellar and intergalactic medium, his cosmological simulations that help illuminate the formation and evolution of structure in the universe, his theoretical contribution to the existence of Dark Matter halos around galaxies, and his dedication to the scientific and academic communities through service as provost, builder of the Sloan Digital Sky Survey and as a mentor of generations of young astronomers.
His work, with students using supernova light curves as calibrated standard candles, has provided evidence for an accelerating expansion of the universe. The dark energy inferred from this result is one of the deepest mysteries of modern science.
For his visionary scientific and technical advancements that have been critical to the fields of helioseismology, asteroseismology, and the emerging field of spectroscopy of transiting exoplanets, and for his critical role in helping a new generation of scientists and facilities to succeed.
For her many important contributions to the field of molecular astrophysics and astrochemistry. Bringing together theoretical chemistry, laboratory studies, and astronomical observations with many instruments, Ewine van Dishoeck has advanced our knowledge of interstellar processes, and of the physical conditions in star-forming regions and protoplanetary disks.