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Universe (Notre univers) is a 1960 black-and-white documentary short film made in 1960 by Roman Kroitor and Colin Low for the National Film Board of Canada (NFB). The NFB writes: "[The film] creates on the screen a vast, awe-inspiring picture of the universe as it would appear to a voyager through space.
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The Cartoon History of the Universe II – From the Springtime of China to the Fall of Rome (Volumes 8–13). Doubleday. p. 305. ISBN 0-385-42093-5. Gonick, Larry (2002). The Cartoon History of the Universe III – From the Rise of Arabia to the Renaissance (Volumes 14–19). Doubleday. p. 300. ISBN 0-393-32403-6. Gonick, Larry (2006).
The Black Hole Era is defined as "40 < n < 100". In this era, according to the book, organized matter will remain only in the form of black holes. Black holes themselves slowly "evaporate" away the matter contained in them, by the quantum mechanical process of Hawking radiation. By the end of this era, only extremely low-energy photons ...
The Sun; Sirius A with Sirius B, a white dwarf; the Crab Nebula, a remnant supernova; A black hole (artist concept); Vela Pulsar, a rotating neutron star; M80, a globular cluster, and the Pleiades, an open star cluster; The Whirlpool galaxy and Abell 2744, a galaxy cluster; Superclusters, galactic filaments and voids
Flammarion had been apprenticed at the age of twelve to an engraver in Paris and it is believed that many of the illustrations for his books were engraved from his own drawings, probably under his supervision. Therefore, it is plausible that Flammarion himself created the image, though the evidence for this remains inconclusive.
The Universe book cover (2nd edition, 2007).. Universe: The Definitive Visual Guide is a 528-page, non-fiction book by nine British co-authors (Robert Dinwiddie, Philip Eales, David Hughes, Iain Nicolson, Ian Ridpath, Giles Sparrow, Pam Spence, Carole Stott and Kevin Tildsley) with a short Foreword by Sir Martin Rees, first published in 2005.
A-type star In the Harvard spectral classification system, a class of main-sequence star having spectra dominated by Balmer absorption lines of hydrogen. Stars of spectral class A are typically blue-white or white in color, measure between 1.4 and 2.1 times the mass of the Sun, and have surface temperatures of 7,600–10,000 kelvin.
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