Messier 92

{{Infobox globular cluster | name = Messier 92 | image = | caption = Pusat dari M92 oleh HST; 1.44′ pandangan | credit = | epoch = J2000 | class = IV^[1] | constellation = Hercules | ra = 17^j 17^m 07.39^d^[2] | dec = +43° 08′ 09.4″^[2] | dist_ly = 267 kly (82 kpc)^[3] | appmag_v = +6.3^[4] Gugusan ini secara terpisah ditemukan oleh Charles Messier pada 18 Maret, 1781 dan dimasukkan dalam urutan ke 92 pada katalognya.^[5] M92 berjarak sekitar 26.700 tahun cahaya jauhnya dari Bumi.

Messier 92 dengan teleskop amatir

Messier 92 dengan menggunakan Isaac Newton Group of Telescopes

Messier 92 adalah salah satu gugusan bola yang paling terang dibelahan Bumi utara, tetapi Messier 92 sering terlewatkan oleh atronom amatir karena kedekatannya terhadap Messier 13 yang lebih spektakuler. Messier 92 dapat dilihat dengan mata telanjang pada kondisi yang sangat bagus.^[6]

Referensi

↑ Shapley, Harlow; Sawyer, Helen B. (1927), "A Classification of Globular Clusters", Harvard College Observatory Bulletin, 849 (849): 11–14, Bibcode:1927BHarO.849...11S.
1 2 Goldsbury, Ryan; et al. (2010), "The ACS Survey of Galactic Globular Clusters. X. New Determinations of Centers for 65 Clusters [ Erratum: 2011AJ....142...66G ]", The Astronomical Journal, 140 (6): 1830–1837, arXiv:1008.2755, Bibcode:2010AJ....140.1830G, doi:10.1088/0004-6256/140/6/1830
↑ Chen, C. W.; Chen, W. P. (2010), "Morphological Distortion of Galactic Globular Clusters", The Astrophysical Journal, 721 (2): 1790–1819, Bibcode:2010ApJ...721.1790C, doi:10.1088/0004-637X/721/2/1790
↑ Kanas, Nick (2007), Star maps: history, artistry, and cartography, Springer-Praxis books in popular astronomy, Springer, hlm. 180, ISBN 0387716688 Kesalahan pengutipan: Parameter dalam tag <ref> tidak sah;
↑ Garfinkle, Robert A. (1997), Star-Hopping: Your Visa to Viewing the Universe, Cambridge University Press, hlm. 131, ISBN 0521598893
↑ Frommert, Hartmut; Kronberg, Christine (September 2, 2007), "Messier 92", SEDS, The Munich Astro Archive, diarsipkan dari asli tanggal 2016-03-04, diakses tanggal 2012-04-08
"SIMBAD Astronomical Database". Results for NGC 6341. Diakses tanggal 2006-11-17.
Paust, Nathaniel E. Q.; Chaboyer, Brian; Sarajedini, Ata (2007), "BVI Photometry and the Luminosity Functions of the Globular Cluster M92", The Astronomical Journal, 133 (6): 2787–2798, arXiv:astro-ph/0703167, Bibcode:2007AJ....133.2787P, doi:10.1086/513511
Forbes, Duncan A.; Bridges, Terry (2010), "Accreted versus in situ Milky Way globular clusters", Monthly Notices of the Royal Astronomical Society, 404 (3): 1203–1214, arXiv:1001.4289, Bibcode:2010MNRAS.404.1203F, doi:10.1111/j.1365-2966.2010.16373.x.
Marks, Michael; Kroupa, Pavel (2010), "Initial conditions for globular clusters and assembly of the old globular cluster population of the Milky Way", Monthly Notices of the Royal Astronomical Society, 406 (3): 2000–2012, arXiv:1004.2255, Bibcode:2010MNRAS.406.2000M, doi:10.1111/j.1365-2966.2010.16813.x. Mass is from M_PD on Table 1.

Pranala luar

Messier 92 di WikiSky: DSS2, SDSS, GALEX, IRAS, Hidrogen α, X-Ray, Astrophoto, Peta langit, Artikel dan gambar
Messier 92 @ SEDS Messier pages Diarsipkan 2004-09-02 di Wayback Machine.
Messier 92, Galactic Globular Clusters Database page
Merrifield, Michael. "M92 – Globular Cluster". Deep Space Videos. Brady Haran.

Koordinat: 17^h 17^m 07.27^s, +43° 08′ 11.5″

[hcob849_11-1] Shapley, Harlow; Sawyer, Helen B. (1927), "A Classification of Globular Clusters", Harvard College Observatory Bulletin, 849 (849): 11–14, Bibcode:1927BHarO.849...11S.

[aj140_6_1830-2] 1 2 Goldsbury, Ryan; et al. (2010), "The ACS Survey of Galactic Globular Clusters. X. New Determinations of Centers for 65 Clusters [ Erratum: 2011AJ....142...66G ]", The Astronomical Journal, 140 (6): 1830–1837, arXiv:1008.2755, Bibcode:2010AJ....140.1830G, doi:10.1088/0004-6256/140/6/1830

[apj721_2_1790-3] Chen, C. W.; Chen, W. P. (2010), "Morphological Distortion of Galactic Globular Clusters", The Astrophysical Journal, 721 (2): 1790–1819, Bibcode:2010ApJ...721.1790C, doi:10.1088/0004-637X/721/2/1790

[kanas2007-4] Kanas, Nick (2007), Star maps: history, artistry, and cartography, Springer-Praxis books in popular astronomy, Springer, hlm. 180, ISBN 0387716688 Kesalahan pengutipan: Parameter dalam tag <ref> tidak sah;

[garfinckle1997-5] Garfinkle, Robert A. (1997), Star-Hopping: Your Visa to Viewing the Universe, Cambridge University Press, hlm. 131, ISBN 0521598893

[maa-6] Frommert, Hartmut; Kronberg, Christine (September 2, 2007), "Messier 92", SEDS, The Munich Astro Archive, diarsipkan dari asli tanggal 2016-03-04, diakses tanggal 2012-04-08

[simbad-7] "SIMBAD Astronomical Database". Results for NGC 6341. Diakses tanggal 2006-11-17.

[aj133_6_2787-8] Paust, Nathaniel E. Q.; Chaboyer, Brian; Sarajedini, Ata (2007), "BVI Photometry and the Luminosity Functions of the Globular Cluster M92", The Astronomical Journal, 133 (6): 2787–2798, arXiv:astro-ph/0703167, Bibcode:2007AJ....133.2787P, doi:10.1086/513511

[mnras404_3_1203-9] Forbes, Duncan A.; Bridges, Terry (2010), "Accreted versus in situ Milky Way globular clusters", Monthly Notices of the Royal Astronomical Society, 404 (3): 1203–1214, arXiv:1001.4289, Bibcode:2010MNRAS.404.1203F, doi:10.1111/j.1365-2966.2010.16373.x.

[mnras406_3_2000-10] Marks, Michael; Kroupa, Pavel (2010), "Initial conditions for globular clusters and assembly of the old globular cluster population of the Milky Way", Monthly Notices of the Royal Astronomical Society, 406 (3): 2000–2012, arXiv:1004.2255, Bibcode:2010MNRAS.406.2000M, doi:10.1111/j.1365-2966.2010.16813.x. Mass is from M_PD on Table 1.

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