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The combination of data from multiple telescopes revealed that the swirling arms of Messier 106 are streams of shock waves and superheated gas.
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Subsequent images from other telescopes revealed that the afterglow faded far more gradually than expected.
Scientists may finally be able to figure that out, thanks to the most extensive online database of early refracting telescopes, revealed at the meeting.
Decent telescopes reveal its cloud-banded disc, currently 41 arcsec wide, while binoculars show up to four of its main moons.
Infrared images from the Keck and Gemini telescopes reveal three giant planets orbiting counterclockwise around a young star, in a scaled-up version of our solar system.
NASA's Spitzer Space Telescope revealed the disk's imprint in a mere 20 seconds.
In the Starry Messenger, Galileo reported that stars appeared as mere blazes of light, essentially unaltered in appearance by the telescope, and contrasted them to planets, which the telescope revealed to be discs.
But shortly thereafter, in his letters on sunspots, he reported that the telescope revealed the shapes of both stars and planets to be "quite round".
Other interferometric studies with multiple telescopes, operating in the infrared, have imaged and confirmed this phenomenon.
Optical interferometry, which has matured within the last two decades, combines the light of multiple telescopes so that exquisitely precise measurements can be made, akin to what might be accomplished with a single, much larger telescope.
But new images taken from the Hubble Telescope reveal a different picture.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com