description W50 Nebula Overview
W50, also called the Manatee Nebula, is a large radio-bright supernova remnant in the constellation Aquila. The compact binary system SS 433, commonly described as a microquasar, lies within the remnant and produces powerful bipolar jets. Those jets interact with the surrounding remnant and contribute to its two-lobed, manatee-like appearance in radio images. The object is studied across radio and X-ray wavelengths because it combines supernova-remnant material with ongoing jet activity.
help W50 Nebula FAQ
Why is W50 called the Manatee Nebula?
W50 is nicknamed the Manatee Nebula because its extended radio and optical structure resembles the shape of a manatee. It is a supernova remnant in the constellation Aquila.
What is SS 433's connection to the W50 Nebula?
W50 hosts SS 433, a bizarre microquasar whose powerful outflows have shaped the surrounding remnant. This connection makes W50 more than a passive cloud of debris, because the central object continues to influence its structure.
Is W50 a planetary nebula or a supernova remnant?
W50 is a supernova remnant, not a planetary nebula. Its association with SS 433 and its location in Aquila are central parts of why astronomers study it.
Where in the sky can the W50 Nebula be found?
The W50 Nebula is located in the constellation Aquila. Searches for it often use the name Manatee Nebula or the associated microquasar SS 433 because both labels point to the same unusual system.
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