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MACS1149-JD

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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.

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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 sections
Contents
  • 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.

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