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Pavo is a constellation in the southern sky whose name is Latin for ' peacock '.Pavo first appeared on a 35-cm (14 in) diameter celestial globe published in 1598 in Amsterdam by Petrus Plancius and Jodocus Hondius and was depicted in Johann Bayer's star atlas Uranometria of 1603, and was likely conceived by Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman.
The RAF insisted that all of the stars must have names, so new names were invented. Alpha Pavonis was named "Peacock" ('pavo' is Latin for 'peacock') whilst Epsilon Carinae was called "Avior". [9] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) [10] to catalog and standardize proper names for stars.
NGC 6744 (also known as Caldwell 101 or the Pavo Galaxy [3]) is an intermediate spiral galaxy in the constellation Pavo (Peacock). Its velocity with respect to the cosmic microwave background is 802 ± 3 km/s, which corresponds to a Hubble distance of 38.6 ± 2.7 Mly (11.82 ± 0.83 Mpc). [1]
NGC 6752 (also known as Caldwell 93 and nicknamed the Great Peacock Globular [7]) is a globular cluster in the constellation Pavo. [8] It is the fourth-brightest globular cluster in the sky, after Omega Centauri, 47 Tucanae and Messier 22, respectively. It is best seen from June to October in the Southern Hemisphere. [9]
This is the list of notable stars in the constellation Pavo, sorted by decreasing brightness. Name B ... Peacock, Joo Tseo; suspected ... "Identification of a ...
Based on the work of Xu Guangqi and the German Jesuit missionary Johann Adam Schall von Bell in the late Ming dynasty, [1] this constellation has been classified as one of the 23 Southern Asterisms (近南極星區, Jìnnánjíxīngōu) under the name Peacock (孔雀, Kǒngqiāo). Peacock (Alpha Pavonis) is the brightmest star in this ...
Phi 2 Pavonis (φ 2 Pav, φ 2 Pavonis) is a solitary [7] star in the southern constellation of Pavo (the Peacock). It is faintly visible to the naked eye with an apparent visual magnitude of +5.10. [2] Based upon an annual parallax shift of 40.55 mas as seen from Earth, it is located 80.4 light years from the Sun.
HD 181433 is a star with a system of orbiting exoplanets located in the southern constellation of Pavo (the Peacock).With an apparent visual magnitude of 8.40, [1] it is too faint to be visible to the naked eye.