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  2. Classical Cepheid variable - Wikipedia

    en.wikipedia.org/wiki/Classical_Cepheid_variable

    As the period increases, the location of the bump moves closer to the maximum and may cause a double maximum, or become indistinguishable from the primary maximum, for stars having periods around 10 days (e.g. Zeta Geminorum). At longer periods the bump can be seen on the ascending branch of the light curve (e.g. X Cygni), [17] but for period ...

  3. Rotation period (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Rotation_period_(astronomy)

    In astronomy, the rotation period or spin period[ 1 ] of a celestial object (e.g., star, planet, moon, asteroid) has two definitions. The first one corresponds to the sidereal rotation period (or sidereal day), i.e., the time that the object takes to complete a full rotation around its axis relative to the background stars (inertial space).

  4. Cepheid variable - Wikipedia

    en.wikipedia.org/wiki/Cepheid_variable

    Cepheid variable. RS Puppis, one of the brightest known Cepheid variable stars in the Milky Way galaxy. (Hubble Space Telescope) A Cepheid variable (/ ˈsɛfi.ɪd, ˈsiːfi -/) is a type of variable star that pulsates radially, varying in both diameter and temperature. It changes in brightness, with a well-defined stable period and amplitude.

  5. AVN Award for Female Performer of the Year - Wikipedia

    en.wikipedia.org/wiki/AVN_Award_for_Female...

    It represents the female porn star who has had the best body of work in the previous year. It has been given annually since 1993. Tori Black was the first two-time winner, winning back-to-back in 2010 and 2011. [1] [2] Angela White was the first three-time winner, winning back-to-back-to-back in 2018, 2019 and 2020. [3]

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    You can find instant answers on our AOL Mail help page. Should you need additional assistance we have experts available around the clock at 800-730-2563.

  7. List of stars with resolved images - Wikipedia

    en.wikipedia.org/wiki/List_of_stars_with...

    Hubble – GHRS [1] 1995: First star with a resolved image outside the Solar System. Sheliak β Lyr Aa 0.46: 6: 960 ± 50: CHARA array – MIRC [25] 2007: Both Aa1 and Aa2 are visible in the animation. θ 1 Ori C: 0.2: 10.6 ± 1.5: 1400: Very Large Telescope – AMBER [26] 2009: In the image, the right inset is θ 1 Ori C and the left inset is ...

  8. SX Phoenicis variable - Wikipedia

    en.wikipedia.org/wiki/SX_Phoenicis_variable

    An SX Phoenicis variable is a type of variable star. These stars exhibit a short period pulsation behavior that varies on time scales of 0.03–0.08 days (0.7–1.9 hours). They have spectral classifications in the range A2-F5 and vary in magnitude by up to 0.7. [ 2 ] Compared to the Sun, these stars have a lower metallicity, which means they ...

  9. DirecTV has a new free streaming service coming. Here's what ...

    www.aol.com/directv-free-streaming-coming-heres...

    DirecTV will launch MyFree DirecTV, a new free streaming TV service, in November. It will have free live TV channels and on-demand shows with ads. DirecTV has a new free streaming service coming.