![]() V 372 Orionis is about 6.41 times bigger than the Sun in radius. Moreover, it does not have any known exoplanets orbiting it perhaps due to their size, which may be challenging to spot compared to smaller stars that can easily be detected. That also means it is within the Milky Way galaxy but not within the Solar System since there is only one star in it, which is the Sun. ![]() Nonetheless, it is within its boundaries. READ ALSO: Hubble Space Telescope Detects 'Ghost Light' From Wandering Stars Scattered Across the Cluster About V 372 OrionisĪs per an article in the Universe Guide, V 372 Orionis is a Subgiant Star in the Orion constellation, although it is not part of the constellation outline. On the other hand, the diffraction spikes of the NASA/ESA/CSA James Webb Space Telescope (JWST) are six-pointed due to Webb's hexagonal mirror segments and three-legged secondary mirror support system. These visible artifacts are caused by starlight interacting with Hubble's inner workings, and they provide indications of Hubble's structure as a result.įour vanes within Hubble support the telescope's secondary mirror, which creates the four spikes encircling the stars in this view. The diffraction spikes encircling the brilliant stars are Hubble's faint imprint on the celestial photograph of the stars. Orion Variables are frequently connected with diffuse nebulae, and V 372 Orionis is no exception the Orion Nebula's patchy gas and dust saturate the image. Both stars are located in the Orion Nebula, a massive star formation zone 1,450 light-years from Earth.Īstronomers can see irregular brightness from these newborn stars as they go through some turbulent mood swings and growing pains. SciTech Daily reports that the brilliant V 372 Orionis, a particular type of variable star called Orion Variable, is featured at the center of the image along with a tiny companion star in the upper left corner. Both are located in the Orion Nebula, a massive area of star formation located 1450 light years away from Earth. This Hubble Space Telescope image features the bright variable star V 372 Orionis and its smaller companion in the upper left. The diffraction spikes of the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope, on the other hand, are six-pointed as a result of Webb’s hexagonal mirror segments and 3-legged support structure for the secondary mirror.Ĭredit: European Space Agency (ESA)/Hubble & NASA, J. The four spikes surrounding the stars in this image are created by four vanes inside Hubble supporting the telescope’s secondary mirror. These prominent artefacts are created by starlight interacting with Hubble’s inner workings, and as a result they reveal hints of Hubble’s structure. Hubble also left its own subtle signature on this astronomical portrait in the form of the diffraction spikes surrounding the bright stars. Data from the Advanced Camera for Surveys and Wide Field Camera 3 at infrared and visible wavelengths were layered to reveal rich details of this corner of the Orion Nebula. ![]() This image overlays data from two of Hubble’s instruments. Orion Variables are often associated with diffuse nebulae, and V 372 Orionis is no exception the patchy gas and dust of the Orion Nebula pervade this scene. These young stars experience some tempestuous moods and growing pains, which are visible to astronomers as irregular variations in luminosity. V 372 Orionis is a particular type of variable star known as an Orion Variable. The background is covered nearly completely by gas: smoky, bright blue gas around the larger star in the center and lower-right, and wispier red gas elsewhere. Small red stars with short diffraction spikes are scattered around them. Image Description: Two very bright stars with cross-shaped diffraction spikes are prominent: the larger is slightly lower-right of center, the smaller lies towards the upper-left corner.
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