NGC 6505
NGC 6505 | |
---|---|
![]() NGC 6505 imaged by Euclid, with LEDA 2678036 (lower left) and LEDA 2678425 (upper right) | |
Observation data | |
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] |
Mass | (2.51 ± 0.06) × 1010[3] M☉ |
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 |
![](http://up.wiki.x.io/wikipedia/commons/thumb/3/33/NGC6505.jpg/310px-NGC6505.jpg)
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]
Altieri's lens
[edit]![](http://up.wiki.x.io/wikipedia/commons/thumb/3/3e/Close-up_of_the_Einstein_ring_around_galaxy_NGC_6505_ESA506346.jpg/220px-Close-up_of_the_Einstein_ring_around_galaxy_NGC_6505_ESA506346.jpg)
The lens was discovered by Euclid Archive Scientist Bruno Altieri in data from ESA's Euclid telescope. The researchers therefore suggest the nickname "Altieri's lens". The discovery was made with early testing data from September 2023, which was out of focus. Later Euclid imaged the galaxy and the lensed galaxy with both the VIS and NIS instruments. The lens was also observed with resolved spectroscopy of the Keck Cosmic Web Imager (KCWI) and the Dark Energy Spectroscopic Instrument (DESI). The lensed galaxy has a redshift of 0.4058 ± 0.003, or 4.46 billion light-years.[3][6]
See also
[edit]References
[edit]- ^ a b c d e f "Results for object NGC 6505". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 11 February 2025.
- ^ a b c SEDS: NGC 6505
- ^ a b c d e O’Riordan, C. M.; Oldham, L. J.; Nersesian, A.; Li, T.; Collett, T. E.; Sluse, D.; Altieri, B.; Clément, B.; Vasan, K. G. C.; Rhoades, S.; Chen, Y.; Jones, T.; Adami, C.; Gavazzi, R.; Vegetti, S. (2025-02-01). "Euclid: A complete Einstein ring in NGC 6505". Astronomy & Astrophysics. 694: A145. doi:10.1051/0004-6361/202453014. ISSN 0004-6361.
- ^ Seligman
- ^ Knud Jahnke (2025-02-10). "Euclid finds complete Einstein Ring in NGC galaxy". Euclid Consortium. Euclid Consortium. Retrieved 2025-02-10.
- ^ "Euclid discovers a stunning Einstein ring". www.esa.int. Retrieved 2025-02-10.
External links
[edit]- "NGC 6505". SIMBAD. Retrieved 2019-08-07.
- "NGC 6505". DSO Browser. Retrieved 2016-08-07.
- Auke Slotegraaf. "NGC 6505". Deep Sky Observer's Companion. Retrieved 2016-08-07.