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  2. Glory (optical phenomenon) - Wikipedia

    en.wikipedia.org/wiki/Glory_(optical_phenomenon)

    Glory around the shadow of a plane. The position of the glory's centre shows that the observer was in front of the wings. A glory is an optical phenomenon, resembling an iconic saint's halo around the shadow of the observer's head, caused by sunlight or (more rarely) moonlight interacting with the tiny water droplets that comprise mist or clouds.

  3. The Intelligent Man's Guide to Science - Wikipedia

    en.wikipedia.org/wiki/The_Intelligent_Man's_Guide...

    The Intelligent Man's Guide to Science received positive reviews from the physicist Derek J. de Solla Price in Science and Floyd C. Gale in Galaxy Science Fiction, [15] and a mixed review from John Pfeiffer in The New York Times.

  4. Near-rectilinear halo orbit - Wikipedia

    en.wikipedia.org/wiki/Near-rectilinear_halo_orbit

    A halo orbit is a periodic, three-dimensional orbit associated with one of the L 1, L 2 and L 3 Lagrange points. Near-rectilinear means that some segments of the orbit have a greater curvature than those of an elliptical orbit of the same maximum diameter, and other segments have a curvature less than that of an elliptical orbit of the same ...

  5. Halo (optical phenomenon) - Wikipedia

    en.wikipedia.org/wiki/Halo_(optical_phenomenon)

    A circumscribed halo (outer ring) together with a comparatively rare 9° halo (inner ring), caused by pyramidal ice crystals. Midsland, the Netherlands, 2019. 22° halo around the Sun, above VBHC Serene Town at Bangalore, India, on May 24, 2021, at 12:15 pm

  6. Galactic halo - Wikipedia

    en.wikipedia.org/wiki/Galactic_halo

    The stellar halo is a nearly spherical population of field stars and globular clusters.It surrounds most disk galaxies as well as some elliptical galaxies of type cD.A low amount (about one percent) of a galaxy's stellar mass resides in the stellar halo, meaning its luminosity is much lower than other components of the galaxy.

  7. Galactic bulge - Wikipedia

    en.wikipedia.org/wiki/Galactic_bulge

    Galactic halo – Spherical component of a galaxy which extends beyond the main, visible component; Galactic corona – Hot, ionised, gaseous component in the Galactic halo; Galaxy formation and evolution – Subfield of cosmology; Mass deficit – Lack of stellar mass in the centers of galaxies

  8. Virial mass - Wikipedia

    en.wikipedia.org/wiki/Virial_mass

    In astrophysics, the virial mass is the mass of a gravitationally bound astrophysical system, assuming the virial theorem applies. In the context of galaxy formation and dark matter halos, the virial mass is defined as the mass enclosed within the virial radius of a gravitationally bound system, a radius within which the system obeys the virial theorem.

  9. Spiral galaxy - Wikipedia

    en.wikipedia.org/wiki/Spiral_galaxy

    Unlike the galactic disc, the halo seems to be free of dust, and in further contrast, stars in the galactic halo are of Population II, much older and with much lower metallicity than their Population I cousins in the galactic disc (but similar to those in the galactic bulge). The galactic halo also contains many globular clusters.