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2. Queue (hairstyle) - Wikipedia

   en.wikipedia.org/wiki/Queue_(hairstyle)

   Napoleon himself, initially wearing long hair tied in a queue, changed his hairstyle and cut his hair short while in Egypt in 1798. [102] However, hair policy in the French army was not uniform; some regiments such as the Imperial Guard foot grenadiers stuck to queues long afterwards, while the 2nd Line Infantry kept their queues as late as 1812.

3. Milky Way - Wikipedia

   en.wikipedia.org/wiki/Milky_Way

   The Milky Way [c] is the galaxy that includes the Solar System, with the name describing the galaxy's appearance from Earth: ...

4. List of largest cosmic structures - Wikipedia

   en.wikipedia.org/wiki/List_of_largest_cosmic...

   Contains the Milky Way, and is the first galaxy filament to be discovered. (The first LQG was found earlier in 1982.) A new report in 2014 confirms the Milky Way as a member of the Laniakea Supercluster. CfA2 Great Wall (1989) 750,000,000: Also known as the Coma Wall. Saraswati Supercluster: 652,000,000 [22]

5. Orders of magnitude (length) - Wikipedia

   en.wikipedia.org/wiki/Orders_of_magnitude_(length)

   Average thickness of Milky Way Galaxy [43] (1,000 to 3,000 ly by 21 cm observations [44]) 10 20: 100 Em: 113.5 Em Thickness of Milky Way Galaxy's gaseous disk [45] 10 21: 1 zettameter (Zm) 1.54 Zm Distance to SN 1987A, the most recent naked eye supernova 1.62 Zm Distance to the Large Magellanic Cloud (a dwarf galaxy orbiting the Milky Way) 1.66 Zm

6. Fifth Season Takes Global Distribution Rights to ... - AOL

   www.aol.com/fifth-season-takes-global...

   Fifth Season has nabbed global distribution rights to the Greek teen drama series “Milky Way,” an eight-part coming-of-age story centered on an unwanted pregnancy that’s written and directed ...

7. No-hair theorem - Wikipedia

   en.wikipedia.org/wiki/No-hair_theorem

   The no-hair theorem was originally formulated for black holes within the context of a four-dimensional spacetime, obeying the Einstein field equation of general relativity with zero cosmological constant, in the presence of electromagnetic fields, or optionally other fields such as scalar fields and massive vector fields (Proca fields, etc.).