Fasciculus:Keck-UCLA Galactic Center Group Sagittarius A* 2022.gif

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Keck-UCLA_Galactic_Center_Group_Sagittarius_A*_2022.gif(500 × 500 elementa imaginalia, magnitudo fasciculi: 4.37 megaocteti, typus MIME: image/gif, looped, 600 repla, 40 s)

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Summarium

Descriptio
English: An animation of the stellar orbits in the central 0.5 arcsec. Images taken from the years 1995 through 2016 are used to track specific stars orbiting the proposed black hole at the center of the Galaxy.

These orbits, and a simple application of Kepler's Laws, provide the best evidence yet for a supermassive black hole, which has a mass of 4 million times the mass of the Sun.

Especially important is the star S0-2 as it has has been observed for more than one full orbital period, which is only 16.17 years.
Datum
Fons https://galacticcenter.astro.ucla.edu/assets/img/animations/2022_animation.mp4
Auctor This animation was created by Prof. Andrea Ghez and her research team at UCLA and are from data sets obtained with the W. M. Keck Telescopes.

Potestas usoris

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Captions

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Stellar Orbits in the Central Parsec

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12 Iulii 2023

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Dies/TempusMinutioDimensionesUsorSententia
recentissima06:32, 8 Novembris 2023Minutum speculum redactionis 06:32, 8 Novembris 2023 factae500 × 500 (4.37 megaocteti)GrufoUploaded a work by This animation was created by Prof. Andrea Ghez and her research team at UCLA and are from data sets obtained with the W. M. Keck Telescopes. from https://galacticcenter.astro.ucla.edu/assets/img/animations/2022_animation.mp4 with UploadWizard

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