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Scutum is a small constellation. Its name is Latin for shield , and it was originally named Scutum Sobiescianum by Johannes Hevelius in 1684. Located just south of the celestial equator , its four brightest stars form a narrow diamond shape.
UY Scuti (BD-12°5055) is a red supergiant star, located 5,900 light-years away in the constellation Scutum.It is also a pulsating variable star, with a maximum brightness of magnitude 8.29 and a minimum of magnitude 10.56, which is too dim for naked-eye visibility.
This is the list of notable stars in the constellation Scutum, sorted by decreasing brightness. Name B Var HD HIP RA Dec vis. mag. abs. mag. Dist. Sp. class Notes α Sct:
With a visual magnitude of 6.0, [2] this cluster is visible to the naked eye from a very dark location free of light pollution. Elsewhere, however, the cluster can be observed with small binoculars. [2] NGC 6605 is located approximately 3.1 degrees southwest of Gamma Scuti, a magnitude 4.67 star in the constellation Scutum.
Delta Scuti, Latinized from δ Scuti, is a variable star in the southern constellation Scutum.With an apparent visual magnitude that fluctuates around 4.72, [4] it is the fifth-brightest star in this small and otherwise undistinguished constellation.
R Scuti (R Sct) is a star in the constellation of Scutum. It is a yellow supergiant and is a pulsating variable known as an RV Tauri variable. It was discovered in 1795 by Edward Pigott at a time when only a few variable stars were known to exist. [11]
The cluster is located just to the east of the Scutum Star Cloud midpoint. [7] The Wild Duck Cluster is one of the richest and most compact of the known open clusters. It is one of the most massive open clusters known, and it has been extensively studied. Its age has been estimated to about 316 million years. [5]
Gamma Scuti, Latinized from γ Scuti, is a single, [9] white-hued star in the southern constellation of Scutum. The apparent visual magnitude of 4.67 [2] indicates this is a dim star but visible to the naked eye. Based upon an annual parallax shift of 10.21 mas as seen from Earth, [1] this star is located about 319 light years from the Sun.