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  2. Messier 34 - Wikipedia

    en.wikipedia.org/wiki/Messier_34

    Messier 34 (also known as M34, NGC 1039, or the Spiral Cluster) is a large and relatively near open cluster in Perseus. It was probably discovered by Giovanni Batista Hodierna before 1654 [ 4 ] and included by Charles Messier in his catalog of comet -like objects in 1764.

  3. Orient Watch - Wikipedia

    en.wikipedia.org/wiki/Orient_Watch

    To celebrate 70 years of the Orient Star line, the Orient Star skeleton watch was introduced with a silicon escapement made using Epson's MEMS technology, which has been used in high end Seiko watches since 2009. [16] [17] In 2001 Seiko Epson (one of three core companies of the Seiko Group) became the majority shareholder (52%) of the company ...

  4. Messier 39 - Wikipedia

    en.wikipedia.org/wiki/Messier_39

    Of the 15 brightest components, six form binary star systems; one more is suspected. HD 205117 is a probable eclipsing binary system with a period of 113.2 days that varies by 0.051 in visual magnitude. Both members seem to be subgiants. [10] Within are at least five [11] chemically peculiar stars and ten [12] suspected short-period variable stars.

  5. Messier 93 - Wikipedia

    en.wikipedia.org/wiki/Messier_93

    Fifty-four variable stars have been found in M93, including one slowly pulsating B-type star, one rotating ellipsoidal variable, seven Delta Scuti variables, six Gamma Doradus variables, and one hybrid δ [b] Sct/γ Dor [c] pulsator. [11] Four spectroscopic binary systems within include a yellow straggler component. [12]

  6. Messier 4 - Wikipedia

    en.wikipedia.org/wiki/Messier_4

    One has been found to be a binary star with a pulsar companion, PSR B1620−26 and a planet orbiting it with a mass of 2.5 times that of Jupiter (M J). [12] One star in Messier 4 was also found to have much more of the rare light element lithium than expected. [13] CX-1 Is located in M4. It is known as a possible millisecond pulsar/neutron star ...

  7. Messier 103 - Wikipedia

    en.wikipedia.org/wiki/Messier_103

    Messier 103 (also known as M103, or NGC 581) is a small open cluster of many faint stars in Cassiopeia.It was discovered on 27 March 1781 by Pierre Méchain, but later added as Charles Messier's last deep-sky object in his catalogue.

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