Blue phantoms and red nebulas recorded near γ Cassiopeia

Three faint nebulas were recorded. IC 59 and IC 63 were identified near the multi-star system γ Cassiopeia as the original Ghosts of Cassiopeia, and the origins of the astronomical apparitions remain a mystery.

The facts note 100 hours, three faint nebulas, and a special oxygen filter.

IC 59 and IC 63 are both identified as the original Ghosts of Cassiopeia. They are near γ Cassiopeia, which is described as a multi-star system.

IC 59 and IC 63 glow red. The facts also state that energetic light attributed to γ Cassiopeia makes hydrogen gas glow red.

Objects 1, 2 and 3 are newly discovered. They appear as blue phantoms, and the facts record the presence of ionized oxygen for them.

The facts give possible explanations: γ Cassiopeia may be accumulating material; Object 3 may involve oxygen compressed and heated in a bow shock; Object 1 could be a planetary nebula; and the origins remain a mystery.

For readers tracking the lunar industry, the verified material is astronomical rather than operational. It provides observational details about three faint nebulas, a special oxygen filter, red glow and ionized oxygen.