Planetary Nebula

Messier 97 - The Owl Nebula

The Owl Nebula (also known as Messier 97, M97 or NGC 3587) is a planetary nebula located approximately 2,030 light years away in the constellation Ursa Major. The owl-like appearance is caused by various formed shells expanding away from the central star.
Observation data: J2000.0 epochRight ascension: 11h 14m 47.734sDeclination: +55° 01′ 08.50″Distance: 2,030 lyApparent magnitude (V): 9.9Apparent dimensions (V): 3′.4 × 3′.3Constellation: Ursa Major
Tech Specs: Sky-Watcher Esprit 120ED Telescope, ZWO ASI2600MC camera running at -10F, 239 x 60 second exposures, Sky-Watcher EQ6R-Pro pier mounted, ZWO EAF and ASIAir Pro, processed in PixInisght. Image Date: December 19, 2023. Location: The Dark Side Observatory (W59), Weatherly, PA, USA (Bortle Class 4).

The Crystal Ball Nebula of Taurus - NGC 1514

This planetary nebula is located right on the border of Taurus and Perseus. It is cataloged as NGC 1514 and is also known as the Crystal Ball Nebula. The magnitude, depending on the source, is listed at 10.9.
Observation data: J2000 epochRight ascension: 04h 09m 16.98573sDeclination: +30° 46′ 33.4699″Distance: 1520 lyApparent magnitude (V): 9.27Apparent dimensions (V): 2.2′Constellation: Taurus
Tech Specs: Orion 8” RC Telescope, ZWO ASI2600MC camera running at -10F, 68 x 60 seconds, Celestron CGEM-DX pier mounted, ZWO EAF and ASIAir Pro, processed in DSS and PixInsight. Image Date: January 2, 2024. Location: The Dark Side Observatory (W59), Weatherly, PA, USA (Bortle Class 4).

Planetary Nebula NGC 2022 in Orion

NGC 2022 is a planetary nebula in the constellation of Orion, located at a distance of 8210 light-years from the Sun. 
NGC 2022 is a vast orb of gas in space, cast off by an aging star. The star is visible in the orb's center, shining through the gases it formerly held onto for most of its stellar life. When stars like the Sun grow advanced in age, they expand and glow red. These so-called red giants then begin to lose their outer layers of material into space. More than half of such a star's mass can be shed in this manner, forming a shell of surrounding gas. At the same time, the star's core shrinks and grows hotter, emitting ultraviolet light that causes the expelled gases to glow. This type of object is called, somewhat confusingly, a planetary nebula, though it has nothing to do with planets. The name derives from the rounded, planet-like appearance of these objects in early telescopes. (REF: https://science.nasa.gov/missions/hubble/hubbles-portrait-of-stars-gaseous-glow/)
Observation data: J2000 epochRight ascension: 05h 42m 06.19056sDeclination: +09° 05′ 10.5843″Distance: 8.21 klyApparent magnitude (V): 11.6Apparent dimensions (V): 28″Constellation: Orion
Tech Specs: Orion 8” RC Telescope, ZWO ASI2600MC camera running at -10F, 81 x 60 seconds, Celestron CGEM-DX pier mounted, ZWO EAF and ASIAir Pro, processed in DSS and PixInsight. Image Date: January 31, 2024. Location: The Dark Side Observatory (W59), Weatherly, PA, USA (Bortle Class 4).

The Eskimo Nebula - NGC 2392

This is the planetary nebula called The Eskimo Nebula or NGC 2392. It is a double-shell planetary nebula located in the constellation Gemini. Radial velocity measurements reveal that this diameter of the cloud is growing at a rate of 68 miles per second (Burnham, 1978).
Tech Specs: Orion 8" f/8 Ritchey-Chretien Astrograph Telescope, Celestron CGEM-DX pier mounted, ZWO ASI290MC and ASI071MC-Pro, ZWO AAPlus, ZWO EAF, 54 x 60 seconds at -10C plus darks and flats, stacked in DSS. Image Date: November 6, 2021. Location: The Dark Side Observatory, Weatherly, PA, USA (Bortle Class 4).

The Shrimp Nebula - Sh2-188 

Sh2-188 is a planetary nebula in Cassiopeia. It does not have an official name but is often called the "Shrimp Nebula" or even the "Dolphin Nebula" due to its shape. The expanding gas from the planetary nebula is colliding with ambient gas in the interstellar medium. The nebula is nearly circular in shape but is much brighter to the southeast (lower right) because the central star is moving rapidly in that direction. Faint wisps of gas can also be seen in the opposite direction. 
Tech Specs: Sky-Watcher Esprit 120ED Telescope,  ZWO AS2600mc-Pro running at 0C, Sky-Watcher EQ6R-Pro mount, Optolong L-eNhance filter (2”), 35 x 300 second exposures, guided using a ZWO 30mm f/4 mini guide scope and ZWO 120 Mini, focus with a ZWO EAF, controlled with a ZWO ASIAir Pro. Processed using PixInsight and DSS. Image Date: August 18, 2022. Location: The Dark Side Observatory, Weatherly, PA, USA (Bortle Class 4).

Planetary Nebula IC1295 in Scutum

IC 1295 is a planetary nebula located in the constellation Scutum.  IC 1295 is a small, green nebula with a low magnitude of 12.7. It is made up of multiple envelopes of gas surrounding a low luminosity star (white dwarf) at the end of its life.
Observation data: J2000 epochRight ascension: 18h 54m 37.206sDeclination: −08° 49′ 39.08″Distance: 4700 lyApparent magnitude (V): 12.7Apparent dimensions (V): 1.7 × 1.4 arcminConstellation: Scutum
Tech Specs: Sky-Watcher Esprit 120ED Telescope, ZWO ASI2600MC camera running at 0F, 54x60 seconds guided exposures, Sky-Watcher EQ6R-Pro pier mounted, ZWO EAF and ASIAir Pro, processed in DSS and PixInsight. Image Date: August 11, 2023. Location: The Dark Side Observatory (W59), Weatherly, PA, USA (Bortle Class 4).