What looks as if it is going to swallow the great Pillars of Creation?
The Eagle Nebula
(M16)
is not a bird, a plane, or
Superman.
M16 is actually a combination of several celestial objects.
NGC 6611
is the young star cluster that appears to peak out beneath the Eagle’s “wings”. The
ultraviolet
light from these stars
ionizes
the surrounding gas, creating the
emission nebula
IC 4703. The
Stellar Spire
is seen reaching towards the Pillars of Creation from the left. Both are structures of cold gas and
dust
that are optimal for
star formation.
Some astronomers previously thought the Pillars of Creation had been
evaporated away by a supernova.
Because M16 is 6,000
light years
away, we would not be able to see the Pillars’ destruction for thousands more years. However, there is no conclusive
evidence of the theorized supernova, so the Pillars of Creation will likely continue to create stars for
millions of years.
Astronomy.co.uk Star Naming Service
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Th Sky Tonight - May 2025
https://www.astronomy.co.uk/the-sky-tonight/
The Pinwheel Galaxy -NASA
The first Full Moon of 2022, known as the Wolf Moon, will occur tonight! Throughout cold January nights, the howling of wolves could be heard around villages in both Europe and America, so the January Full Moon became widely known as the Wolf Moon.
The exact time of the Full Wolf Moon is January 17, 2022, 23:48 GMT
The Lagoon Nebula - Hubble
This is a small section of the Cygnus supernova blast wave which appears as a delicate streak of light.
Credit: ESA/Hubble & NASA, W. Blair; acknowledgment: Leo Shatz
An exploding star !
Hubble
The station crew sees 16 sunrises a day, and they officially started 2022 at 12am GMT.
The Snow Angel Nebula - Hubble
Crescent Earth
The Earth as seen from the Moon on the Command Module of Apollo17 on December 16, 1972.
Credit: @NASA (image #AS17-152-23274); Processing: @JPMajor
Dolphin head nebula located near the center of the constellation Canis Major
DEM L249, located in the Large Magellanic Cloud, is an unusual supernova remnant.
Image Credit: NASA, ESA, and Y. Chou (Academia Sinica, Institute of Astronomy and Astrophysics); Processing: Gladys Kober (NASA/Catholic University of America)
