Tutorial for "Orion Nebula" Interactive The Orion Nebula is one of the nearest locations in our galaxy where stars are being formed now. You can see it with your own eyes: a faint, fuzzy patch of light just below the belt in the constellation of Orion. The visible portion is just a tiny portion of the entire Orion Molecular Cloud complex, most of which is hidden from our view by thick layers of dust and gas. You have seen several illustrations of the Orion Nebula in this section, but it may help for you to take a tour through a three-dimensional model of the visible section of the Nebula. This lab gives you several different ways to investigate the region. When you start the lab, you will see a picture frame with controls on the right. At the bottom right is a toggle switch, which starts in the "Explorer" position. In this mode, you may look at a portion of the Nebula from different points of view. Begin with the "Full View," which shows most of the visible portions of the cloud. Move the cursor into the picture, so that the cursor turns into a small hand. Then click and hold the left mouse button while dragging the mouse. The view will rotate, as if you were flying around the cloud. As you move, look carefully at the stars scattered around you. Do you see any which look fuzzy, or dirty? What are they? Clicking on the "Trapezium" button will give you a close-up look at the four bright stars near the center of the Nebula (as shown by the red box in the thumbnail picture at upper right in the frame). Like all stars in the Nebula, these are very young, no more than a few million years old. All four members of the Trapezium are more massive than our Sun. The brightest of the four, called "theta Orionis C", is the hottest, largest, and brightest of all. It provides most of the ultraviolet light which excites the gas in the Nebula, causing it to glow. The greenish color is produced by atoms of oxygen which have had two of their eight electrons knocked away by ultraviolet photons. Clicking on the "Proplyd" button will show you a close-up view of one the many proplyds (protoplanetary disks) in the Orion Nebula. The location of this particular proplyd is shown by the red box in the thumbnail picture at upper right in the frame. Each proplyd contains a very young star, surrounded by a disk of gas. The star and disk together are surrounded by a dense shell of material, a remnant of the cloud which collapsed to form the star. Notice how dense and dusty the disk is -- it blocks much of the light which passes freely through the cloud around it. This proplyd is shaped like a teardrop, as are a number of others in the Nebula. Something appears to be pushing the gas on one side. Can you figure out the source of this "wind" in space? If you move the toggle switch at lower right to "Guided Tour", you will see a movie showing the view as a spaceship flies through the Orion Nebula.