A mysterious, yawning mouth of gas and dust gives Caldwell 9 its popular nickname, the Cave Nebula. The nebula is actually part of a much larger cloud of gas and dust called Cepheus B, named after its home constellation, Cepheus. This image of Caldwell 9, captured by Hubble’s Wide Field and Planetary Camera 2, shows just a small portion of the
nebula near the mouth of the cave.Roughly 3,000 light-years away and lying in the plane of our Milky Way galaxy, the Cave Nebula is an
emission nebula, formed of gases that emit their own light. The bright arc that forms the mouth of the cave is an active birthplace for stars, known as an
H II region, where hot clouds of atomic hydrogen have become
ionized.Though boasting a
magnitude of about 8 and a span of roughly 40 light-years, Caldwell 9 is a diffuse and low-contrast object, so it can still be difficult to find in the sky. Its first known notation, in fact, was not until 1959 after astronomer Stewart Sharpless captured it on photographic plates and included it as the 155th object in his second catalog of H II regions, giving Caldwell 9 its alternate catalog name, Sh2-155.Caldwell 9 is tantalizing to researchers because, according to radio and near-infrared studies of this nebula, the area is bursting with young, hot stars popping into existence. Investigating such regions of star birth helps astronomers learn more about how stars begin their lives. Hubble’s Wide Field and Planetary Camera 2 imaged this region of Caldwell 9 in 1995 to search for signs of planet-forming disks around young stars in the nebula, similar to disks Hubble had previously spotted in the
Orion Nebula (M42). (NASA)
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