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Stars and stellar evolution
Peering through a dense cocoon of dust in the Carina Nebula

These two images of a huge pillar of star birth demonstrate how observations taken in visible and in near-infrared light by NASA’s Hubble Space Telescope reveal dramatically different and complementary views of an object.

The pictures demonstrate one example of the broad wavelength range of the new Wide Field Camera 3 (WFC3), extending from ultraviolet to visible to near-infrared light. WFC3 was installed aboard Hubble in May 2009 during Servicing Mission 4.

Near-infrared image of Carina sees through dust

Observations taken in different wavelengths reveal different features. Top image (taken in visible light) shows the huge pillar of gas and dust in Carina. Bottom image (taken in near-infrared light) penetrates the wall of gas and dust to reveal the fledgling stars inside, including one that is shooting jets to the left and right.

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Composed of gas and dust, the pillar resides in a tempestuous stellar nursery called the Carina Nebula, located 7,500 light-years away in the southern constellation Carina. The pair of images shows that astronomers are given a much more complete view of the pillar and its contents when distinct details not seen at visible wavelengths alone are uncovered in near-infrared light.

The top image, taken in visible light, shows the tip of the 3-light-year-long pillar, bathed in the glow of light from hot, massive stars off the top of the image. Scorching radiation and fast winds (streams of charged particles) from these stars are sculpting the pillar and causing new stars to form within it. Streamers of gas and dust can be seen flowing off the top of the structure.

Nestled inside this dense structure are fledgling stars. They cannot be seen in this image because they are hidden by a wall of gas and dust. Although the stars themselves are invisible, one of them is providing evidence of its existence. Thin puffs of material can be seen traveling to the left and to the right of a dark notch in the center of the pillar. The matter is part of a jet produced by a young star. Farther away, on the left, the jet is visible as a grouping of small, wispy clouds. A few small clouds are visible at a similar distance on the right side of the jet. Astronomers estimate that the jet is moving at speeds of up to 1,400,000 kilometers per hour (850,000 miles per hour). The jet’s total length is more than 15 light-years.

In the image at bottom, taken in near-infrared light, the dense column and the surrounding greenish-colored gas all but disappear. Only a faint outline of the pillar remains. By penetrating the wall of gas and dust, the near-infrared vision of WFC3 reveals the infant star that is probably blasting the jet. Part of the jet nearest the star is more prominent in this view. These features can be seen because infrared light, unlike visible light, can pass through the dust.

Other infant stars inside the pillar also appear to emerge. Three examples are the bright star almost directly below the jet-producing star, a fainter one to its right, and a pair of stars at the top of the pillar. Winds and radiation from some of the stars are blowing away gas from their neighborhoods, carving out large cavities that appear as faint dark holes.


"Tales of … Peering through a dense cocoon of dust in the Carina Nebula" describes a pillar of gas and dust within which stars are forming. Visible light cannot penetrate the dust but the near-infrared image shows us what is happening. The two images complement each other and provide a more complete story of stellar birth.

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10-12, but the material can be adapted for use in other grades at the teacher's discretion
How to use in the classroom

Teachers can use this resource as:

A content reading selection. Teachers should discuss the meaning of unfamiliar vocabulary prior to having students read this selection.

An engagement activity. Have students read the selection. Ask them to describe how the visible and near-infrared images complement each other.

An inquiry tool. Propose a question, such as, "How do astronomers know stars are forming deep inside the pillar?" Have students read the selection and write down as many questions as they can about the information in the text.

A source of information. Students can describe the characteristics of star formation within the pillar and then research whether astronomers see similar characteristics in other pillars using Hubble press releases.

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