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Garlic nebula Abell 85 (EXPLORED)
Abell 85 Supernova Remnant, also known as CTB 1, is a large supernova remnant and one of the prominent astronomical objects that reveal the remnants of stellar explosions in our galaxy. Here are more detailed insights about this unique object:
Abell 85 is a supernova remnant (SNR), meaning it is the result of a massive star explosion after it exhausted its nuclear fuel. The star that exploded was in its final stages of life, ending with a colossal blast that scattered material into space.
The nebula is located in the constellation Cassiopeia and is approximately 10,000 light-years away from us.
Abell 85 appears as a large spherical bubble of gas and cosmic dust. It is characterized by a diffuse luminous ring, formed by the interaction of the ejected material from the explosion with the surrounding interstellar medium.
In astrophotography, this remnant is visible through emission lines of heavier elements such as ionized hydrogen (Hα), as well as the glow from doubly ionized oxygen ([O III]).
The estimated age of Abell 85 is around 10,000 years. This suggests that the supernova explosion occurred thousands of years ago, gradually leaving behind this beautiful, expanding gas structure.
This supernova remnant belongs to the Type II Supernova class, where a massive star explodes due to the collapse of its core. Heavier elements like iron and nickel that formed during the explosion now contribute to the material we observe in the nebula today.
Supernovae play a vital role in the evolution of galaxies by dispersing heavy elements into space, which are crucial for forming planets and life.
Stellar explosions like the one that created Abell 85 are also a significant source of accelerated cosmic rays, which are high-energy particles that travel through the galaxy.
Abell 85 is not just an ordinary supernova remnant, but a window into the ancient epochs of the universe, offering us an opportunity to reflect on how stars and planets evolve within our galaxy.
Ha 93 x 300” (7hr 45min)
Sii 96 x 300” (8hr 00min)
RGB 30 x 10” (0hr 15min)
Oiii 175 x 300” (14hr 35min)
Oiii 71x600” (11hr 50min)
Total integration time - (42hr 25min)
Gears:
M: CQ350
T: Sharpstar 15028HNT
C: ZWO ASI 2600MM Pro
F: Antlia
Garlic nebula Abell 85 (EXPLORED)
Abell 85 Supernova Remnant, also known as CTB 1, is a large supernova remnant and one of the prominent astronomical objects that reveal the remnants of stellar explosions in our galaxy. Here are more detailed insights about this unique object:
Abell 85 is a supernova remnant (SNR), meaning it is the result of a massive star explosion after it exhausted its nuclear fuel. The star that exploded was in its final stages of life, ending with a colossal blast that scattered material into space.
The nebula is located in the constellation Cassiopeia and is approximately 10,000 light-years away from us.
Abell 85 appears as a large spherical bubble of gas and cosmic dust. It is characterized by a diffuse luminous ring, formed by the interaction of the ejected material from the explosion with the surrounding interstellar medium.
In astrophotography, this remnant is visible through emission lines of heavier elements such as ionized hydrogen (Hα), as well as the glow from doubly ionized oxygen ([O III]).
The estimated age of Abell 85 is around 10,000 years. This suggests that the supernova explosion occurred thousands of years ago, gradually leaving behind this beautiful, expanding gas structure.
This supernova remnant belongs to the Type II Supernova class, where a massive star explodes due to the collapse of its core. Heavier elements like iron and nickel that formed during the explosion now contribute to the material we observe in the nebula today.
Supernovae play a vital role in the evolution of galaxies by dispersing heavy elements into space, which are crucial for forming planets and life.
Stellar explosions like the one that created Abell 85 are also a significant source of accelerated cosmic rays, which are high-energy particles that travel through the galaxy.
Abell 85 is not just an ordinary supernova remnant, but a window into the ancient epochs of the universe, offering us an opportunity to reflect on how stars and planets evolve within our galaxy.
Ha 93 x 300” (7hr 45min)
Sii 96 x 300” (8hr 00min)
RGB 30 x 10” (0hr 15min)
Oiii 175 x 300” (14hr 35min)
Oiii 71x600” (11hr 50min)
Total integration time - (42hr 25min)
Gears:
M: CQ350
T: Sharpstar 15028HNT
C: ZWO ASI 2600MM Pro
F: Antlia