Amateur astronomers make significant contributions to the field of astronomy, and their observations of variable stars serve as a valuable asset to the profession. Variable stars are celestial objects that exhibit periodic changes in brightness, and their study provides critical insights into stellar properties, evolution, and the larger universe. Amateur astronomers, with their passion and increasingly advanced equipment, offer a unique set of advantages in this domain, complementing the work of professional astronomers and expanding our understanding of these fascinating objects. One of the key advantages of amateur astronomers observing variable stars is their sheer numbers. The global community of amateur stargazers is vast, and their collective efforts result in a continuous stream of observations. This extensive dataset complements the work of professional astronomers, enabling them to monitor more variable stars than they could alone. The collaboration between amateurs and

NGC 7635 - The Bubble Nebula processed by Brian Puhl from image data acquired on Insight Observatory's CDK500 remote telescope located in Spain (AFIL-7). NGC 7635, commonly known as the Bubble Nebula, is one of the most fascinating and visually striking objects in our night sky. Situated in the constellation Cassiopeia, this celestial wonder is a massive emission nebula, and its nickname is derived from its distinctive bubble-like appearance. The Bubble Nebula is particularly renowned for its unique characteristics, which have captivated the curiosity of astronomers and stargazers alike. One of the most distinctive features of the Bubble Nebula is the enormous, nearly spherical shell of gas and dust that envelops a central, massive star named BD+60°2522. This star's intense ultraviolet radiation ionizes the surrounding hydrogen gas, causing it to emit a brilliant red glow, typical of emission nebulae. The expanding shell of the Bubble Nebula, created by the powerful solar