Hubble Finds Life and Death in the Universe

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Image Credit & Copyright: NASA/ESA Hubble Space Telescope.

Images like these are some of my favorite in all the night sky. Here we see the beautiful globular star cluster New General Catalog 1846 (NGC 1846) in the southern constellation Dorado, which, means I’ve never seen this with my own eyes….bummer.

Not only is this cluster in Dorado, it lies outside of the Milky Way 160,000 light years away in the Large Magellanic Cloud (LMC), a satellite galaxy to our home galaxy. Now, like many objects in the universe, things can be easy to miss and or overlook and at first glance, this is often the case here when not accompanied by an enlarged box which highlights the feature. At 6 o’clock down “below” the cluster you see a beautiful emerald colored planetary nebula. It’s not known if this stellar remnant is a member of the cluster or just a line of sight object but it’s movement in relation to other stars within the group lead astronomers to believe that it is home in the cluster.

WHAT IS A PLANETARY NEBULA?

As for the objects themselves they are very low density and comprised of mostly gaseous materials. They range in size depending on the mass of the dying star, composition, speed of material ejection and the amount of time the event has been taking place as well as under what processes it was undergoing while it was being formed. Density in PN’s are so low (Approximately a million atoms per cubic centimeter) that no vacuum on Earth can recreate these conditions. Though planetary nebulae were known about for over 200 years, nobody knew what they were or what their origins were besides the fact that they could look and see them.

Inside the core of a star, pressures and temperatures are so great that a process called Thermo-Nuclear Fusion can take place. It’s important to remember that stars don’t “burn” as burning is a chemical reaction. Thermo-Nuclear Fusion is a nuclear reaction. Hydrogen atoms are being fused together to create helium atoms. When the two nuclei fuse together the combined mass is slightly less than the sum of the original nuclei and the difference is released as energy. As the progenitor star burns through all of its available fuel the star quickly begins to die. The key word here is “available” fuel as most of the hydrogen in a star will never be fused in the core. When this happens gravity begins to win over the outward pressure of the nuclear reaction. The star then begins to crush down onto itself from the extreme inward pressure that gravity is now imposing on it.

Ironically enough, this very process of compression causes the core to become super-heated. Core temperatures rise to ten-times the temperature they were while in the main sequence phase. Once the temperature reaches 180,000,000 degrees the temperature will be hot enough to fuse helium into carbon. As this continues, the star will begin to quickly use up its available helium fuel. The massive temperatures cause the star to swell and the asymptotic giant branch aka, the infamous red giant phase begins. Vast layers or shells of gas are then released into the surrounding cosmos creating what’s known as proto-planetary or pre-planetary nebula (PPN’s). The furiously hot star whose inner layers are now exposed radiate massive amounts of ultraviolet radiation rendering the surrounding material aglow and that’s where the planetary nebula (PN) phase begins.

When the available helium begins to run dry, gravity once again begins to take over, and again the star is crushed in upon itself; this time down to about the size of the Earth. It is at this point when electron degeneracy pressure is enabled. This means that electrons themselves are being crushed together so tightly that their repulsive pressure on one another will hold the star up. That is where it will remain for billions of years as a white dwarf.

Most stars in the universe (about 95%) will end their lives this way; the rest will die as supernovae.

NAME: NGC 1846.

WHAT IS IT?: Globular star cluster with planetary nebula.

HOW FAR AWAY IS IT?: Roughly 160,000 light years.

HOW BIG IS IT?: Roughly 100 light years in diameter.

APPARENT MAGNITUDE: A pretty dim 11.

WHERE IS IT? (General): Constellation Dorado.

WHERE IS IT? (Exact RA/DEC J2000): R.A. 05h 07m 33s.94 / Dec. -67° 27′ 41″.29.

NASA Hubblesite News Center page for this image: http://hubblesite.org/newscenter/archive/releases/2011/35/image/a/

SIMBAD data on this object: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC++1846

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Image | This entry was posted in Astronomy (Learning), Astrophotography (DSOs), Images, Nebula (Planetary), Star Clusters (Globular-Open) and tagged , , , , , , , , , , , . Bookmark the permalink.

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