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  2. NGC 4622 - Wikipedia

    en.wikipedia.org/wiki/NGC_4622

    Analysis of a color-age star formation angle sequence of the Fourier components establishes that the strong outer pair is the leading pair A Fourier component image of the arm pairs is shown with one of the pair of arms marked for the newly discovered inner CCW pair (black dots) as well as one of the already known (CW) outer pair (white dots).

  3. MC Skat Kat - Wikipedia

    en.wikipedia.org/wiki/MC_Skat_Kat

    MC Skat Kat was created by Michael Patterson and performed by the Wild Pair duo of Bruce DeShazer and Marv Gunn on "Opposites Attract". MC Skat Kat's rap was written and performed by Derrick Stevens, although Romany Malco, who did the majority of the writing for the M.C. Skat Kat & the Stray Mob album, is often mistakenly credited for being the voice of the rap on Opposites Attract, a story ...

  4. Binary system - Wikipedia

    en.wikipedia.org/wiki/Binary_system

    The most common kinds of binary system are binary stars and binary asteroids, but brown dwarfs, planets, neutron stars, black holes and galaxies can also form binaries. A multiple system is similar but consists of three or more objects, for example triple stars and triple asteroids (a more common term than 'trinary').

  5. Sigma Octantis - Wikipedia

    en.wikipedia.org/wiki/Sigma_Octantis

    Sigma Octantis is a solitary [9] star in the Octans constellation that forms the pole star of the Southern Hemisphere.Its name is also written as σ Octantis, abbreviated as Sigma Oct or σ Oct, and it is officially named Polaris Australis (/ p oʊ ˈ l ɛər ɪ s ɔː ˈ s t r eɪ l ɪ s /). [10]

  6. XAUUSD - Wikipedia

    en.wikipedia.org/?title=XAUUSD&redirect=no

    Download QR code; Print/export Download as PDF; Printable version; In other projects Appearance. move to sidebar hide. ... XAUUSD. Add languages ...

  7. Co-orbital configuration - Wikipedia

    en.wikipedia.org/wiki/Co-orbital_configuration

    (or 1:-1 if orbiting in opposite directions). [1] There are several classes of co-orbital objects, depending on their point of libration. The most common and best-known class is the trojan, which librates around one of the two stable Lagrangian points (Trojan points), L 4 and L 5, 60° ahead of and behind the larger body respectively.

  8. Mu1 Scorpii - Wikipedia

    en.wikipedia.org/wiki/Mu1_Scorpii

    The two stars revolve each other along a circular orbit with the components separated by 12.9 times the Sun's radius. [3] Due to occultation of each component by the other, the apparent magnitude of the system decreased by 0.3 and 0.4 magnitudes over the course of the binary's orbit, which takes 34 hours 42.6 minutes to complete.

  9. HD 40873 - Wikipedia

    en.wikipedia.org/wiki/HD_40873

    HD 40873 is a star in the northern constellation of Auriga, a few degrees to the south of Delta Aurigae.Located around 455 light-years distant, [1] it shines with a luminosity approximately 38 times that of the Sun and has an effective temperature of 7,753 K. [6] It is a suspected variable star [2] and has a fairly rapid rotation rate, showing a projected rotational velocity of 134 km/s. [7]