This article is about the band of dark areas in the night-sky running along the Milky Way. Not to be confused with the particular dark nebula called Dark River of the Rho Ophiuchi cloud complex.
In dark, clear night skies, the rift appears as clear as the bright bulge of stars around the Galactic Center does to the naked eye or binoculars. The rift is largely between the Solar System (which is close to the inner edge of the Orion Arm) and the next arm, inward, the Sagittarius Arm. The clouds are an obstruction to millions of the galaxy's stars detected at visible wavelengths, which compose a bright hazy band appearing 30° wide and arching through the night sky. The clouds within our radial sector of the galaxy span about 800–1,000 parsecs (2,600–3,300 ly) from Earth.[1] The clouds are estimated to contain about 1 million solar masses of plasma and dust.[2]
^Green, Gregory M; Schlafly, Edward F; Finkbeiner, Douglas P; Rix, Hans-Walter; Martin, Nicolas; Burgett, William; Draper, Peter W; Flewelling, Heather; Hodapp, Klaus; Kaiser, Nicholas; Kudritzki, Rolf Peter; Magnier, Eugene; Metcalfe, Nigel; Price, Paul; Tonry, John; Wainscoat, Richard (2015). "A Three-Dimensional Map of Milky Way Dust". The Astrophysical Journal. 810 (1): 25. arXiv:1507.01005. Bibcode:2015ApJ...810...25G. doi:10.1088/0004-637X/810/1/25. S2CID55653509.