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  2. Number the Stars - Wikipedia

    en.wikipedia.org/wiki/Number_the_Stars

    18947847. LC Class. PZ7.L9673 Nu 1989. Number the Stars is a work of historical fiction by the American author Lois Lowry about the escape of a family of Jews from Copenhagen, Denmark, during World War II. The story revolves around ten-year-old Annemarie Johansen, who lives with her mother, father, and sister Kirsti in Copenhagen in 1943.

  3. Stellar classification - Wikipedia

    en.wikipedia.org/wiki/Stellar_classification

    A number following a comma is a scale between 1 and 9 based on the ratio of ZrO and TiO. A number following a slash is a more-recent but less-common scheme designed to represent the ratio of carbon to oxygen on a scale of 1 to 10, where a 0 would be an MS star. Intensities of zirconium and titanium may be indicated explicitly. Also occasionally ...

  4. Star system - Wikipedia

    en.wikipedia.org/wiki/Star_system

    Artist's impression of the orbits of HD 188753, a triple star system. A star system or stellar system is a small number of stars that orbit each other, [1] bound by gravitational attraction. A large group of stars bound by gravitation is generally called a star cluster or galaxy, although, broadly speaking, they are also star systems.

  5. Stellar parallax - Wikipedia

    en.wikipedia.org/wiki/Stellar_parallax

    Stellar parallax is the basis for the parsec, which is the distance from the Sun to an astronomical object that has a parallax angle of one arcsecond. (1 AU and 1 parsec are not to scale, 1 parsec = ~206265 AU) Stellar parallax is the apparent shift of position (parallax) of any nearby star (or other object) against the background of distant ...

  6. AR Lacertae - Wikipedia

    en.wikipedia.org/wiki/AR_Lacertae

    At the distance of AR Lac, this is equivalent to a projected separation of about 930 AU. It has a mass of 0.6 +0.04 −0.09 M ☉ and a radius of 0.0125 +0.0014 −0.0012 R ☉. The companion has an estimated age of 5.75 Gyr and has been steadily cooling for about the last 1.62 Gyr. As a main sequence star, it had a mass of 1.34 +0.46 −0.27 M

  7. Polaris - Wikipedia

    en.wikipedia.org/wiki/Polaris

    In 2018 Polaris was 0.66° (39.6 arcminutes) away from the pole of rotation (1.4 times the Moon disc) and so revolves around the pole in a small circle 1.3° in diameter. It will be closest to the pole (about 0.45 degree, or 27 arcminutes) soon after the year 2100. [ 35 ]

  8. Magnitude (astronomy) - Wikipedia

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

    Stars that have magnitudes between 1.5 and 2.5 are called second-magnitude; there are some 20 stars brighter than 1.5, which are first-magnitude stars (see the list of brightest stars). For example, Sirius is magnitude −1.46, Arcturus is −0.04, Aldebaran is 0.85, Spica is 1.04, and Procyon is 0.34. Under the ancient magnitude system, all of ...

  9. Flamsteed designation - Wikipedia

    en.wikipedia.org/wiki/Flamsteed_designation

    Flamsteed designation. A Flamsteed designation is a combination of a number and constellation name that uniquely identifies most naked eye stars in the modern constellations visible from southern England. They are named for John Flamsteed who first used them while compiling his Historia Coelestis Britannica. (Flamsteed used a telescope, [1] and ...