The last phase of a given star
To look and to observe are synonyms of actions, but when it comes to Astronomy they are not the same matter. Observing is more than just simply looking at something, but trying to understand what that something is and how amazing it is to be able to see it. People less involved with astronomy would consider the views from my binocular as something boring and repetitive because many objects seem to look the same: fuzzes and faints spots in the sky. Yet it is those white-grayish spots of light that make my stargazing sessions the most exciting adventures in the night.
Looking at galaxies, nebulas or stars that are thousands or millions of light years from us is an indescribable experience, no matter how they look in the eyepiece. Of course getting more visual detail is even more exciting, but knowing what they are, how big they should be or how far away they are and seeing them with your own eyes in a live view is a priceless experience that should be done at least once in a lifetime.
Wherever there is a star or at least a main sequence star like our sun, it could be a planetary nebula eventually in time. After having spent their primary fuel, hydrogen and start to burn Helium instead, a main sequence star becomes a red giant star because several physical changes in the nucleus. Sometime later (speaking in thousands or millions of years) the star begins to use heavier elements to get energy such as oxygen and carbon and it experiences violent changes in temperature, pressure and gravity causing the ejection of the outer layers of the star while the core becomes a large mass compacted nucleus: a white dwarf. This stellar spectacle is known as planetary nebulae. There is nothing involving planets in this matter, it is simply a “misnamed object” coming from the German astronomer William Herschel, who compared this phenomenal view with the images provided at the time of the gas giants in our own solar system.
M27 was the first planetary Nebula to be discovered by Charles Messier in 1764. It seemed in the binoculars as if it was a dense circle which was cut by two parallel and opposite segments. Those segments, better seen with averted vision, apparently complete the circular shape but they seemed dim and fuzzy so it was difficult to see the edges of the nebular zone. The core itself seemed brighter and denser than an average globular cluster and the edges of the core were well defined. In most of the photos pictured on the web it is possible to see two big lobules around the tiny white star showing the color of the excited particles by the radiation of the dying star.
Watching this dying star was an amazing experience, to know that not only could I look into a global cluster and see the birthplace of stars, but look into a planetary nebulae and see the end of this ball of fire’s life.
Once again, I wish you clear and dark skies!
Edited by: Jennifer Steinberg (editor in chief)