Astronomers used the Hubble Space Telescope to zoom in for a close-up look at one sliver of the Cygnus Loop nebula—a huge bubble of glowing gasses. They found gossamer filaments resembling lines in a wrinkled bedsheet stretched across two light-years. This region lies at the outer edge of the expanding bubble, and was produced by an exploding star 20,000 years ago.
Analyzing the shock wave's location, astronomers found that the filaments haven't slowed down at all in the last 20 years of Hubble observations, and they haven't changed shape. The material is speeding into interstellar space at over half a million miles per hour—fast enough to travel from Earth to the Moon in less than half an hour.
Credits
Image
NASA, ESA, STScI
About The Object | |
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Object Name | Cygnus Loop |
Object Description | Supernova Remnant |
R.A. Position | 20:56:04.18 |
Dec. Position | 31:56:25.90 |
Constellation | Cygnus |
Distance | 2500 light-years |
Dimensions | Image is about 2.4 arcmin across (about 1.74 light-years) |
About The Data | |
Data Description | The HST observations include those from program: 15893 (R. Sankrit) |
Instrument | WFC3/UVIS |
Exposure Dates | July 1, 2020 |
Filters | F502N, F656N |
About The Image | |
Color Info | These images are a composite of separate exposures acquired by the The Hubble Space Telescope using the WFC3/UVIS instrument. Two filters were used to sample narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Cyan: F502N, Orange: F656N |
Compass Image |
About The Object | |
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Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
Object Description | The type of astronomical object. |
R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
Distance | The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs. |
Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
About The Data | |
Data Description |
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Instrument | The science instrument used to produce the data. |
Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
Filters | The camera filters that were used in the science observations. |
About The Image | |
Image Credit | The primary individuals and institutions responsible for the content. |
Publication Date | The date and time the release content became public. |
Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |