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Night Flight to the Stars

Activity 4A: Mapping a Birth Cloud

The Omega Nebula (M17) is a cloud of gas and dust, which can be seen with binoculars. This object lies just above the "teapot" of the Omega Nebula (M17)

Sagittarius in the general direction of the center of our Galaxy. It's a relatively nearby region of active star formation and is very bright at infrared wavelengths.

The bright stars which light up the visible nebula also warm an invisible cloud of dust to the right of the visible nebula. The warm dust has a temperature of around 100K (-173°C or -279°F) near the stars and drops to 40K (-233°C or -387°F) farther out. Farther out is a very large cloud of cold gas which receives very little radiation.

In M17 hot young stars have formed near the surface of an interstellar cloud. The energy emitted by these stars has created a "blister" on the cloud surface. The bright nebula seen above is a side view of this blister. The dark cloud lies to the right of the visible nebula in this view.

The square in the corner of this photo represents the field of the KAO telescope. Choose other places where you might look for warm invisible gas. Mark the places where the KAO astronomers choose to gather data during the flight. Record the brightness levels that they report. Use the brightest visible stars as your reference. image from lower left coner of M17
Image is 2° × 2°
The IRAS infrared imaging satellite produced this image of M17 (the brightest feature in this image: Beyond it is Milky Way.) Notice the warm areas to the west of the bright star cloud. Use this image in deciding where you might collect data from the KAO.
This page was created by Daniel Helfman, a junior at Mission San Jose High School in Fremont, CA.


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