This NASA Hubble Space Telescope image reveals a pair of one-half light-year long interstellar twisters (eerie funnels and twisted rope structures) in the heart of the Lagoon Nebula, which lies 5,000 light-years away in the direction of the constellation Sagittarius. The central hot star, Herschel 36 (lower right), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Other hot stars, also present in the nebula, are ionizing the extended optical nebulosity. The ionizing radiation induces photo-evaporation of the surfaces of the clouds and drives away violent stellar winds tearing into the cool clouds. This is similar to tornadoes on Earth. The large difference in temperature between the hot surface and cold interior of the clouds, combined with the pressure of starlight, may produce strong horizontal shears to twist the clouds into their tornado-like appearance. The Lagoon Nebula and nebulae in other galaxies are sites where new stars are being born from dusty molecular clouds. These regions are the "space laboratories" for the astronomers to study how stars form and the interactions between the winds from stars and the gas nearby. By studying the wealth of data revealed by HST, astronomers will understand better how stars form in the nebulae.
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