An Enigmatic Astronomical Explosion
A bright young star is surrounded by a shroud of thick gas and dust in this image from the NASA/ESA Hubble Space Telescope. Hubble’s Wide Field Camera 3 inspected a young stellar object, over 9000 light years away in the constellation Taurus, to help astronomers understand the earliest stages in the lives of massive stars. This object — which is known to astronomers as IRAS 05506+2414 — is thought to be an example of an explosive event caused by the disruption of a massive young star system. If so, it would only be the second such example known.
Usually the swirling discs of material surrounding a young star are funnelled into twin outflows of gas and dust from the star. In the case of IRAS 05506+2414, however, a fan-like spray of material travelling at velocities of up to 350 kilometres per second is spreading outwards from the centre of this image.
Astronomers turned to Hubble’s Wide Field Camera 3 to measure the distance to IRAS 05506+2414. While it is possible to measure the velocity of material speeding outwards from the star, astronomers cannot tell how far from Earth the star actually is from a single observation. However, by measuring the distance that the outflow travels between successive images, they will be able to infer the distance to IRAS 05506+2414. This will allow astronomers to determine how bright the star is and how much energy it is emitting, and hence to estimate its mass — all vital information that will help to understand the origin of this bright young star’s unusual outflow.
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Credit:ESA/Hubble & NASA, R. Sahai
About the Image
Id: | potw2238a |
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Type: | Observation |
Release date: | 19 September 2022, 06:00 |
Size: | 1066 x 959 px |
About the Object
Name: | IRAS 05506+2414 |
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Constellation: | Taurus |
Category: | Cosmology |
Wallpapers
Coordinates
Position (RA): | 5 53 43.51 |
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Position (Dec): | 24° 14' 45.82" |
Field of view: | 2.28 x 2.05 arcminutes |
Orientation: | North is 135.7° right of vertical |
Colours & filters
Band | Wavelength | Telescope |
---|---|---|
Infrared YJ | 1.1 μm |
Hubble Space Telescope
WFC3 |
Infrared H | 1.6 μm |
Hubble Space Telescope
WFC3 |
Infrared Fe II | 1.64 μm |
Hubble Space Telescope
WFC3 |
Infrared Fe II continuum | 1.67 μm |
Hubble Space Telescope
WFC3 |