File:Hubble Sees Monstrous Cloud Boomerang Back to our Galaxy (24676686535).jpg

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Hubble Space Telescope astronomers are finding that the old adage “what goes up must come down” even applies to an immense cloud of hydrogen gas outside our Milky Way galaxy.

The invisible cloud is plummeting toward our galaxy at nearly 700,000 miles per hour. Though hundreds of enormous, high-velocity gas clouds whiz around the outskirts of our galaxy, this so-called “Smith Cloud” is unique because its trajectory is well known. New Hubble observations suggest it was launched from the outer regions of the galactic disk, around 70 million years ago. The cloud was discovered in the early 1960s by doctoral astronomy student Gail Smith, who detected the radio waves emitted by its hydrogen.

This composite image shows the size and location of the Smith Cloud on the sky. The cloud appears in false-color, radio wavelengths as observed by the Green Bank Telescope in West Virginia. The visible-light image of the background star field shows the cloud's location in the direction of the constellation Aquila.

Read more: go.nasa.gov/1ZX8Fzo

Credits: Saxton/Lockman/NRAO/AUI/NSF/Mellinger
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Source Hubble Sees Monstrous Cloud Boomerang Back to our Galaxy
Author NASA Goddard Space Flight Center from Greenbelt, MD, USA

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This image was originally posted to Flickr by NASA Goddard Photo and Video at https://flickr.com/photos/24662369@N07/24676686535. It was reviewed on 17 September 2016 by FlickreviewR and was confirmed to be licensed under the terms of the cc-by-2.0.

17 September 2016

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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28 January 2016

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current19:57, 17 September 2016Thumbnail for version as of 19:57, 17 September 20161,200 × 530 (739 KB)Vanished Account ByeznhpyxeuztibuoTransferred from Flickr via Flickr2Commons

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