What is happening inside this unusual nebula?
Planetary nebula Tc 1, captured here in exquisite detail by the James Webb Space Telescope, is the celestial site where buckyballs were first identified in 2010. Buckminsterfullerene — as buckyballs are officially called — is a molecule with 60 carbon atoms (C60) arranged in the shape of a soccer ball. The molecule is named for architect Buckminster Fuller because of its resemblance to the geodesic dome he helped popularize. Webb’s new data reveal where the C60 molecules live in this nebula, and the geometry is striking: they populate a thin spherical shell around the central star, visible here as the bright edge of the nebula’s glowing orange central region. Look closely near the nebula’s heart and a more perplexing feature emerges: a delicate structure shaped uncannily like an upside-down question mark, fitting punctuation for the many questions this nebula still poses.
Astronomy.co.uk Star Naming Service
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Th Sky Tonight - May 2025
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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)
