Explanation: Sometimes the simplest shapes are the hardest to explain. For example, the origin of the mysterious cone-shaped region located just below the center of the above picture remains a mystery. The dark region clearly contains much dust which blocks light from the emission nebula and open cluster NGC 2264 behind it. One hypothesis holds that the cone is formed by wind particles from an energetic source blowing past the Bok globule at the head of the cone.

Information: The Scale of the Universe Debate in April 1996

<<  Mart  >> Pn Vt Sr Cht Pt Sb Vs         1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 1995   1996   1997 1998   1999   2000 2001   2002   2003 2004   2005   2006 2007   2008   2009 2010   2011   2012 2013   2014   2015 2016   2017   2018 2019   2020   2021 2022   2023   2024

Yanvar' Fevral' Mart Aprel' Mai Iyun' Iyul' Avgust Sentyabr' Oktyabr' Noyabr' Dekabr'

Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: nebula - Cone nebula - Mezhzvezdnaya pyl' - emissionnaya tumannost' - Rasseyannoe skoplenie Publikacii so slovami: nebula - Cone nebula - Mezhzvezdnaya pyl' - emissionnaya tumannost' - Rasseyannoe skoplenie
Sm. takzhe: NGC 602: zvezdy protiv stolbov Prizraki v Kassiopee Melott 15 v tumannosti Serdce Tumannost' Tyul'pan i chernaya dyra Lebed' X-1 Triplet v Strel'ce NGC 7789: Roza Karoliny NGC 602: zvezdnoe skoplenie Ustrica Vse publikacii na tu zhe temu >>