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Bok Globules

November 30, 2009 Leave a comment

The birth of a baby is one of the most amazing miracles to behold in the natural world. From conception to birth, the change that a baby endures beginning as a single cell and ending up as a full grown and functioning human being in the short span of forty weeks is unrivaled in nature. Stellar birth, however, is also an extremely amazing event. Although the birth of a star takes an eternity in comparison to the human gestational cycle, it is one of the most amazing processes that occur within the celestial realms. One place where the birth of stars occurs is within dark molecular clouds called Bok Globules.

A pair of Bok Globules

Bok globules are dark, dense clouds of dust and gas found within H II regions, which are low density clouds of gas and plasma that can be as big as several hundred light-years in diameter. These Bok globules typically have a mass that ranges between 0.1 and 2000 solar masses, a unit of astronomical mass measurement that is equal to the mass of the Sun.  They are contained with an area of about a light year or so in diameter. Molecular hydrogen, carbon dioxide, helium, and a small percentage of silicate dust are found within these clouds.

These astronomical phenomena where first observed by astronomer Bart Bok in the 1940s. Bok and his researcher partner E.F. Reilly published a paper in 1947 that stated these clouds were similar to the cocoons of insects. They hypothesized that these clouds were undergoing gravitational collapse to form protostars from which star clusters and star systems were formed. This hypothesis was difficult to verify due to the fact that the clouds obscure all visible light being emitted from within the cloud. However, infrared analysis observations published in 1990 confirmed that stars were being formed within the Bok globules.

Bok globules are the smallest manifestations of dark nebulae, which are interstellar clouds that contain a very high concentration of dust that allows them to scatter and absorb visible light. Bok globules support both the inflow and outflow of material, a process common in the development of protostars. These clouds are known to have a temperature of around 10 Kelvin.

Bok globules are still being intensely researched and their inmost properties are still being analyzed. While there is still much information to be garnered from Bok globules, what is known is that they actually serve as a cocoon protecting infant protostars from being stripped by radioactive stellar winds from other nearby stars and the block all visible light. Bok globules are an amazing phenomena and the understanding of these clouds will give us an even greater insight into the birth of stars.

References

http://astronomy.swin.edu.au/cms/astro/cosmos/B/Bok+Globule

http://www.universetoday.com/2009/02/02/journey-inside-a-bok-globule/

Nebulae: An overview

November 16, 2009 Leave a comment

Pillars of Creation Nebula

A nebula is an interstellar cloud of dust, hydrogen gas, helium gas, and plasma. The word nebula is derived from the Latin word for cloud. Originally the word nebula was used to describe any extended astronomical object including galaxies. The older use of the word survives in modern usage in some confusing ways. Various star clusters and galaxies are still referred to as nebulae. Strictly speaking, the word nebula should be reserved for clouds composed of gas and dust. There are several types of nebulae.

Omega Emission Nebula

The first type of nebula is called an emission nebula. These are clouds of ionized gas that emit various colors. The most common color expressed by an emission nebula is red due to the ionizing hydrogen. There are other colors as well, but none as abundant as red due to the great amount of hydrogen within these clouds. The most common cause for the ionization of the gas is a result of high-energy photons from a nearby hot star, as in the case of emission nebulae located in H II regions where there are new stars being born or dying stars which are in the process of expelling their outer layers exposing the hot core. The majority of emission nebulae are not caused by a single star as the star would have to be massive to ionize a significant part of the cloud. Instead, the ionization occurs due to an entire cluster of high temperature stars.

Witch Head Reflecting Nebula

The next type of nebulae is the reflecting nebula. These are similar to emission nebulae in the regard that they are both visible due to light. Within a reflecting nebula, there is not enough energy to ionize the gas to form an emission nebula. However, there is enough to scatter the light and make the dust within the cloud visible. Therefore, the reflecting nebula takes on the color characteristic of the star that the nebula is reflecting. There are around 500 known reflection nebulae. Many times, emission and reflecting nebulae occur within the same dust cloud where one part of the cloud is hot enough to ionized the gas, but there are sections where the temperature is lower and the light is reflected.

Horse Head Dark Nebula

The final type of nebulae is the dark nebula. A dark nebula is a nebula that is so dense that it obscures the light that attempts to pass through it from emission nebulae or background stars. The extinction of light is caused by the interstellar dust located at the coldest, densest places within the nebula. Large dark nebulae are associated with Giant Molecular Clouds, whereas smaller dark nebulae are called Bok globules. Within these nebulae, stellar events such as the formation of new stars occur as the gravitational forces act within the clouds.

Nebulae offer a spectacular celestial show as they interact with outside energy forces. Much research is still being invested into these phenomena, and the more we discover helps us to discern better the origins of our own corner of the universe.

References

http://astro.nineplanets.org/twn/types.html

http://www.daviddarling.info/encyclopedia/R/reflectionneb.html

http://abyss.uoregon.edu/~js/glossary/dark_nebula.html