Back Messier 19 Afrikaans مسييه 19 Arabic Cúmulu globular M19 AST NGC 6273 Azerbaijani M19 (аб’ект Месье) Byelorussian M19 BE-X-OLD M19 Bulgarian Messier 19 BS Messier 19 Catalan NGC 6273 CE

Messier 19

Messier 19
Globular cluster Messier 19 in Ophiuchus
Observation data (J2000 epoch)
ClassVIII[1]
ConstellationOphiuchus
Right ascension17h 02m 37.69s[2]
Declination−26° 16′ 04.6″[2]
Distance28.7 kly (8.8 kpc)[3]
Apparent magnitude (V)6.8[4]
Apparent dimensions (V)17.0′
Physical characteristics
Mass1.10×106[3] M☉
Radius70 ly
Metallicity = –1.53[5] dex
Estimated age11.90 Gyr[5]
Other designationsNGC 6273, GCl 52[2]
See also: Globular cluster, List of globular clusters

Messier 19 or M19 (also designated NGC 6273) is a globular cluster in the constellation Ophiuchus. It was discovered by Charles Messier on June 5, 1764[6] and added to his catalogue of comet-like objects that same year. It was resolved into individual stars by William Herschel in 1784. His son, John Herschel, described it as "a superb cluster resolvable into countless stars".[7] The cluster is located 4.5° WSW of Theta Ophiuchi and is just visible as a fuzzy point of light using 50 mm (2.0 in) binoculars. Using a telescope with a 25.4 cm (10.0 in) aperture, the cluster shows an oval appearance with a 3′ × 4′ core and a 5′ × 7′ halo.[6]

M19 is one of the most oblate of the known globular clusters.[7] This flattening may not accurately reflect the physical shape of the cluster because the emitted light is being strongly absorbed along the eastern edge. This is the result of extinction caused by intervening gas and dust. When viewed in the infrared, the cluster shows almost no flattening.[8] It lies at a distance of about 28.7 kly (8.8 kpc) from the Solar System,[3] and is quite near to the Galactic Center at only about 6.5 kly (2.0 kpc) away.[9]

This cluster contains an estimated 1,100,000 times the mass of the Sun[3] and it is around 11.9 billion years old.[5] The stellar population includes four Cepheids and RV Tauri variables, plus at least one RR Lyrae variable for which a period is known.[10] Observations made during the ROSAT mission failed to reveal any low-intensity X-ray sources.[11]

Map showing the location of M19
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  3. ^ a b c d Cite error: The named reference apj742_1_51 was invoked but never defined (see the help page).
  4. ^ "Messier 19". SEDS Messier Catalog. Retrieved 21 July 2024.
  5. ^ a b c Cite error: The named reference mnras404_3_1203 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference thompson2007 was invoked but never defined (see the help page).
  7. ^ a b Cite error: The named reference burnham1978 was invoked but never defined (see the help page).
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  11. ^ Cite error: The named reference aaa368_137 was invoked but never defined (see the help page).

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