Category
page 1Musca

Musca
is a small constellation in the deep southern sky. It was one of 12 constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman, and it first appeared on a celestial globe in diameter published in 1597 (or 1598) in Amsterdam by Plancius and Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer's Uranometria of 1603. It was also known as for 200 years. Musca remains below the horizon for most Northern Hemisphere observers.
NGC 5189
planetary nebula in the constellation Musca
NGC 4372
Globular cluster in the constellation Musca
NGC 4833
Globular cluster in the constellation Musca
Hourglass Nebula
planetary nebula in the constellation Musca
NGC 4463
star cluster
NGC 4815
intermediate age open cluster in the inner Galactic disk
Alpha Muscae
star in the constellation Musca
list of stars in Musca
Wikimedia list article
HD 100546
star
Gamma Muscae
star in the constellation Musca
LP 145-141
star in the constellation Musca
TYC 8998-760-1
star in the constellation Musca containing a planetary system
Beta Muscae
star in the constellation Musca
Delta Muscae
star in the constellation Musca
HD 111232
star in the constellation Musca
HD 111232 b
extrasolar planet
Lambda Muscae
star in the constellation Musca
Zeta2 Muscae
star in the constellation Musca
Epsilon Muscae
variable star in the constellation Musca
Theta Muscae
variable star in the constellation Musca
Mu Muscae
variable star in the constellation Musca
S Muscae
variable star in the constellation Musca
BHR 71
Nebula in the constellation Musca
GRS 1124-683
star in the constellation Musca
Eta Muscae
star system in the constellation Musca
HD 103079
binary star system in the constellation Musca
SNR G299.2-02.9
G299.2-2.9 is a supernova remnant in the Milky Way, 16,000 light years from Earth. It is the remains of a Type Ia supernova.
The observed radius of the remnant shell translates to approximately 4,500 years of expansion, making it one of the oldest observed Type Ia supernova remnants.