k Galactic gravitational lensing, ALMA image Galactic gravitational lensing, Atacama Large Millimeter Array ALMA image. The orange ring is millimetre wavelength light from the galaxy SDP.81 12 billion light years distant, gravitationally lensed around a closer galaxy not seen, 4 billion light years distant. The millimetre wavelength light is emitted by dust bright orange ring and carbon monoxide CO, fainter orange areas in the distant galaxy. This galaxy is in the constellation of Hydra. The observations were made in 2014. Stock Photo - Afloimages
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Galactic gravitational lensing, ALMA image Galactic gravitational lensing, Atacama Large Millimeter Array  ALMA  image. The orange ring is millimetre wavelength light from the galaxy SDP.81  12 billion light years distant , gravitationally lensed around a closer galaxy  not seen, 4 billion light years distant . The millimetre wavelength light is emitted by dust  bright orange ring  and carbon monoxide  CO, fainter orange areas  in the distant galaxy. This galaxy is in the constellation of Hydra. The observations were made in 2014.
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Galactic gravitational lensing, ALMA image

Galactic gravitational lensing, Atacama Large Millimeter Array (ALMA) image. The orange ring is millimetre wavelength light from the galaxy SDP.81 (12 billion light years distant), gravitationally lensed around a closer galaxy (not seen, 4 billion light years distant). The millimetre wavelength light is emitted by dust (bright orange ring) and carbon monoxide (CO, fainter orange areas) in the distant galaxy. This galaxy is in the constellation of Hydra. The observations were made in 2014.

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