Contributor
RickStudent, Philosopher, Writer, Developer
c 1915
William Henry Bragg — c 1915
Photo Credit: By Nobel foundation - Public Domain, https://commons.wikimedia.org/w/index.php?curid=33407292
Bohr and Margrethe Nørlund on their engagement in 1910
Photo Credit: Niels Bohr Institute, Public Domain, https://commons.wikimedia.org/w/index.php?curid=24652845
Margrethe Nørlund Bohr
Photo Credit: Public Domain, https://commons.wikimedia.org/w/index.php?curid=24652845
The cake model of the hydrogen atom (Z = 1) or a hydrogen-like ion (Z > 1), where the negatively charged electron confined to an atomic shell encircles a small, positively charged atomic nucleus and where an electron jumps between orbits, is accompanied by an emitted or absorbed amount of electromagnetic energy (hν). The orbits in which the electron may travel are shown as grey circles; their radius increases as n2, where n is the principal quantum number. The 3 → 2 transition depicted here produces the first line of the Balmer series, and for hydrogen (Z = 1) it results in a photon of wavelength 656 nm (red light).
Bohr model - hydrogen atom — The cake model of the hydrogen atom (Z = 1) or a hydrogen-like ion (Z > 1), where the negatively charged electron confined to an atomic shell encircles a small, positively charged atomic nucleus and where an electron jumps between orbits, is accompanied by an emitted or absorbed amount of electromagnetic energy (hν). The orbits in which the electron may travel are shown as grey circles; their radius increases as n2, where n is the principal quantum number. The 3 → 2 transition depicted here produces the first line of the Balmer series, and for hydrogen (Z = 1) it results in a photon of wavelength 656 nm (red light).
Photo Credit: By JabberWok, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=2639910
Bohr model - hydrogen atom The cake model of the hydrogen atom (Z = 1) or a hydrogen-like ion (Z > 1), where the negatively charged electron confined to an atomic shell encircles a small, positively charged atomic nucleus and where an electron jumps between orbits, is accompanied by an emitted or absorbed amount of electromagnetic energy (hν). The orbits in which the electron may travel are shown as grey circles; their radius increases as n2, where n is the principal quantum number. The 3 → 2 transition depicted here produces the first line of the Balmer series, and for hydrogen (Z = 1) it results in a photon of wavelength 656 nm (red light).
Werner Heisenberg (left) with Bohr at the Copenhagen Conference in 1934
Photo Credit: By Fermilab, U.S. Department of Energy - Public Domain, https://commons.wikimedia.org/w/index.php?curid=6877522
Niels Bohr, physicist
Photo Credit: Niels Bohr's Nobel Prize biography, from 1922, Public Domain, https://commons.wikimedia.org/w/index.php?curid=288274
Tao of Physics 1st ed cover
Photo Credit: Scan of book cover, Fair use, https://en.wikipedia.org/w/index.php?curid=46514354
Tao of Physics avatar
Photo Credit:
Fritjof Capra
Photo Credit: By Zenobia Barlow - Donated by the Center for Ecoliteracy with permission for publication. http://www.ecoliteracy.org/, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=14736022
Web of Old Testament Sources
Photo Credit: TREY the Explainer - https://youtu.be/XKp4yWGTfXo?t=433
Field where the Battle of Llantada occurred
Photo Credit: By Valdavia - Own work, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=9500129