Astronomy:IC 2497

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Short description: Spiral galaxy in the constellation Leo Minor
IC 2497
Hannys voorwerp.jpg
IC 2497 with Hanny's Voorwerp by HST
Credit: NASA, ESA, W. Keel (University of Alabama), and the Galaxy Zoo Team
Observation data (J2000.0[1] epoch)
ConstellationLeo Minor [2]
Right ascension 09h 41m 04.076s [1]
Declination+34° 43′ 58.57″ [1]
Redshift0.051633 [1]
Distance650 Mly (199.29 Mpc)
Characteristics
Apparent size (V)0.390' × 0.320' [1]

IC 2497 is a spiral galaxy[3] close to the intergalactic cloud Hanny's Voorwerp.[1] The galaxy is a former quasar, whose light lit up Hanny's Voorwerp, which is now a light echo of that extinct quasar.[4] It is about 45,000–70,000 light-years (14,000–21,000 pc) away from Hanny's Voorwerp.[5] The quasar shut down sometime in the last 70,000 years.[6] This revises current theories of quasar operation, as the quasar is quiescent, shutting down much faster than was thought possible,[7] and is much cooler than predicted.[5] The galaxy is currently 100 to 10,000 times dimmer than it was when its quasar burned into Hanny's Voorwerp.[8]

One supernova has been observed in IC 2497: SN 2020ilb (type Ia, mag. 19) was discovered on 29 April 2020.[9]

References

Further reading

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