The Bubble Nebula (Caldwell 11) is an emission nebula located in the constellation Cassiopeia, approximately 7,100 light-years from Earth. It spans about 7 light-years in diameter. The nebula is famous for its remarkably symmetrical bubble, which is created by the intense stellar wind from the massive, hot central star (SAO 20575). This wind pushes the surrounding interstellar gas into a shell-like structure, while the star’s radiation causes the hydrogen gas to glow with a deep reddish light.
The Salt and Pepper Cluster (M52) is a rich open star cluster located in Cassiopeia, roughly 5,000 light-years away from Earth. It spans about 19 light-years across and contains around 200 stars. Often called the "Salt and Pepper Cluster" due to its dense, speckled appearance, it is a very young cluster, estimated to be only about 35 million years old. While it appears close to the Bubble Nebula in your wide-field photo, it is actually about 2,000 light-years closer to us.
The Lobster Claw Nebula (Sh2-157) is a large emission nebula located on the border between the constellations Cassiopeia and Cepheus, approximately 11,000 light-years away from Earth. It is a vast complex of ionized gas, named for its two prominent filaments that resemble the pincers of a lobster. The nebula's glow is driven by the intense ultraviolet radiation from several massive stars, most notably the rare and incredibly hot Wolf-Rayet star WR 157. It is part of a larger star-forming region that includes the nearby Bubble Nebula, though the Lobster Claw sits much further back in the Perseus Spiral Arm of our galaxy.
The Arrowhead Cluster (NGC7510) is a small but distinct open star cluster located in the constellation Cepheus, roughly 11,400 light-years distant from Earth. It is easily identified by its unique, elongated shape that resembles an arrowhead or a small wedge pointing through the starry background. This cluster is quite young, with its brightest members being hot, blue-white stars. Because of its great distance and the intervening interstellar dust along the plane of the Milky Way, the cluster appears somewhat dimmed and reddened, but it remains a sharp, sparkling feature at the edge of the Lobster Claw's field.