NGC 6505 | |
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![]() NGC 6505 imaged by Euclid, with LEDA 2678036 (lower left) and LEDA 2678425 (upper right) | |
Observation data (J2000 epoch) | |
Constellation | Draco |
Right ascension | 17h 51m 07.4726s[1] |
Declination | +65° 31′ 50.925″[1] |
Redshift | 0.042414 ± 0.0000160[1] |
Heliocentric radial velocity | 12,715±5 km/s[1] |
Distance | 186.55 ± 13.06 Mpc (608.4 ± 42.6 Mly)[1] |
Apparent magnitude (V) | 14.6[2] |
Apparent magnitude (B) | 15.6[2] |
Surface brightness | 14.8 |
Characteristics | |
Type | E-S0[2] |
Size | ~243,300 ly (74.59 kpc) (estimated)[1] |
Apparent size (V) | 1.1′ × 1.0′ |
Other designations | |
2MASX J17510740+6531507, UGC 11026, MCG +11-22-007, PGC 60995, CGCG 322-018 |
NGC 6505 is an elliptical galaxy with Hubble sequence classification E/S0 in the northern celestial hemisphere constellation Draco. It is about 608 million light years away from the Milky Way galaxy and has a diameter of about 190,000 light years. It was discovered on June 27, 1884 by Lewis A. Swift.[4] In 2025, the Euclid Space Telescope found a complete Einstein ring surrounding NGC 6505.[5]
With the help of the lens model some properties of the central region of NGC 6505 were estimated. One result is that the central region has an initial mass function that is heavier than predicted with Chabrier and a dark matter fraction of 11.1+5.4
−3.5 % inside the Einstein radius.[3]
O’Riordan2025
was invoked but never defined (see the help page).
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