NGC 1952, also known as M1, is a planetary nebula located in the constellation of Taurus. It was the first object of its type discovered and studied by French astronomer Charles Messier in 1758. Since then, it has been examined by many researchers and is considered one of the most important and fascinating objects in the observable universe.Planetary nebulae are space objects formed by the expansion and dissolution of the outer layers of a dying star. NGC 1952 is considered one of the brightest and closest planetary nebulae to Earth, making it an ideal object for observations and scientific studies.Visual observation of NGC 1952 shows a crescent-shaped bright form, with a central brightness visibly more luminous. This shape is created by the expanding matter that emits light from the central star, which is visible in ultraviolet observation. X-ray observations revealed the presence of a hot and bright central source, suggesting the presence of a neutron star.Spectroscopic studies of NGC 1952 have also revealed important information on the structure and physical properties of the nebula. Spectra showed the presence of elements such as hydrogen, helium, carbon, and oxygen, as well as trails of dust and gas. Measurements of the nebula's expansion speed have also allowed for the determination of its mass and age, which are estimated to be about 10,000 years and 0.6 solar masses, respectively.Finally, observations of NGC 1952 have also provided information on the complex astrophysical phenomena occurring in planetary nebulae, such as the formation of new stars and the dissipation of surrounding matter. Continuous observations of this object will allow for a better understanding of these phenomena and to learn more about the evolution and death of stars.In conclusion, NGC 1952 is an exceptional scientific object that continues to fascinate researchers and astronomy enthusiasts. The observations and studies of this planetary nebula have led to new discoveries about the universe and the complex astrophysical phenomena that occur within it. It is therefore important to continue observations of NGC 1952 in order to deepen our understanding of this fascinating object.