MACS1149-JD
Sign in to saveMACS1149-JD1 (also known as JD1 and PCB2012 3020) is a young galaxy that is known for being one of the farthest known galaxies from Earth. It was discovered in 2014 and confirmed in 2018. The JD1 galaxy is at a redshift of about z=9.11, or about away from Earth meaning that it formed when the universe was around 500 million years old.
In the Vinony graph
Vinony's link graph records 190 inbound references to MACS1149-JD, and connects out to epoch, Earth and universe.
It sits within the topics Dwarf galaxies and Leo (constellation).
Vinony links it to 13 Wikipedia language editions.
Key facts
- Galaxy.name
- MACS1149-JD1
- Galaxy.image
- Hubble and ALMA image of MACS J1149.5+2223.jpg
- Galaxy.caption
- Hubble and ALMA image of galaxy cluster MACS J1149.5+2223 with an inset of MACS1149-JD1
- Galaxy.epoch
- J2000
- Galaxy.constellation name
- Leo
- Galaxy.dist_ly
- (co-moving) (light travel)
- Galaxy.group_cluster
- MACS J1149.5+2223
- Galaxy.type
- Dwarf
- Galaxy.appmag_v
- 26.8
- Galaxy.size_v
- 0.00075 x 0.00035
- Galaxy.size
- 3,000 ly (diameter)
- Galaxy.names
- [PCB2012] 3020, [KOI2016] HFF4C-YJ1, [ZZI2017] 663
via Wikipedia infobox
Wikidata facts
- Instance of
- galaxy
- Constellation
- Leo
- Image
- Annotated montage - galaxy cluster MACS J1149+2223 and high-z galaxy MACS1149-JD 01.jpg
Show 7 more facts
- apparent magnitude
- 25.80
- right ascension
- 177.3899333
- declination
- 22.4127167
- epoch
- J2000.0
- redshift
- 9.2
- Commons category
- MACS1149-JD1
- radial velocity
- 294084
Sources (1)
via Wikidata · CC0
~1 min read
Encyclopedic overview
3 sectionsContents
- See also
- References
- External links
MACS1149-JD1 (also known as JD1 and PCB2012 3020) is a young galaxy that is known for being one of the farthest known galaxies from Earth. It was discovered in 2014 and confirmed in 2018. The JD1 galaxy is at a redshift of about z=9.11, or about away from Earth meaning that it formed when the universe was around 500 million years old.
The carbon and neon abundances of JD1 are below the solar abundance ratio. The under-abundance of carbon suggests recent star formation where a Type II supernova enriched the interstellar medium (ISM) with oxygen, but intermediate mass stars have not yet enriched the ISM with carbon.
Excerpted from Wikipedia’s “MACS1149-JD” article, available under the CC BY-SA 4.0 licence.