ISOHDFS 27

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search
ISOHDFS 27
ISOHDFS 27 taken by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationTucana
Right ascension22h 32m 47.7s
Declination−60° 33′ 35.9″
Redshift0.5807±0.0003
Heliocentric radial velocity174,090 km/s (108,170 mi/s)
Galactocentric velocity174,009 km/s (108,124 mi/s)
Distancebillion ly (1.8 billion pc) (light travel distance)
billion ly (2.1 billion pc)
(comoving distance)
Apparent magnitude (V)20.51
Characteristics
TypeSab
Mass1.04×1012 M
Size130 kly (40 kpc)
Apparent size (V)0.07 × 0.07
Other designations
HDFS J223247.66-603335.9, LFR2003 193, SB-WF 3572-1508, CDD2000 1670, USNOA2 0225-31548819

ISOHDFS 27 is a spiral galaxy in the constellation Tucana, and was discovered in the Hubble Deep Field South survey. It is the most massive spiral galaxy found in the survey,[1] measuring 130,000 light-years (40,000 parsecs) in diameter.[2] It is located approximately 6 billion light-years (1.8 billion parsecs) from Earth[2] and has a mass greater than 1000 billion times the mass of the Sun, making it about four times as massive as the Milky Way.[1]

It was once thought to be the largest spiral galaxy in the universe,[1] but it has since been dethroned by NGC 6872.[3]

See also

[edit]
[edit]

References

[edit]
  1. ^ a b c "Most Massive Spiral Galaxy Known in the Universe". European Southern Observatory Press Release: 25. 2000-12-01. Bibcode:2000eso..pres...25.
  2. ^ a b information@eso.org. "Massive spiral galaxy ISOHDFS 27". www.eso.org. Retrieved 2023-09-22.
  3. ^ SVS (2013-10-17). "NASA Scientific Visualization Studio | The Largest-Known Spiral Galaxy". SVS. Retrieved 2023-09-22.