This is also a likely explanation for the structure of NGC 5189, although so far only one star has been found in the centre of the nebula. Sometimes this shape is a sphere, sometimes a double cone and sometimes a ring or spiral. Keller, from the University of Sao Paulo in Brazil, also used the Hubble data to study the properties of light and wind emitted by planetary nebulae, including NGC 5189 – a likely explanation for the structure of NGC 5189, although so far only one star has been found at the centre of the nebula. Keller, from the University of Sao Paulo in Brazil, also used Hubble data to study the properties of light and winds emitted by planetary nebulae, including NGC 5189.NGC 5189, also known as a spiral planetary nebula, is located in the constellation Musca about 3,000 light years away.
AURA’s Space Telescope Science Institute in Baltimore, Maryland, is responsible for Hubble’s science operations.
