Samiksha Jaiswal (Editor)

Markarian 421

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Right ascension
  
11 04 27.314

Redshift
  
0.030021

Constellation
  
Declination
  
+38° 12′ 31.80″

Type
  
BL LAC

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Distance
  
397-434 million light-years(122-133 Mpc)

Apparent magnitude (V)
  
12.9 (SIMBAD)13.3 (NED)11.6-16 (B Band)

Similar
  
Markarian 501, BL Lacertae, PKS 2155‑304, 3C 279, 3C 66A

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Markarian 421 (Mrk 421, Mkn 421) is a blazar located in the constellation Ursa Major. The object is an active galaxy and a BL Lacertae object, and is a strong source of gamma rays. It is about 397 million light-years (redshift: z=0.0308 eq. 122Mpc) to 434 million light-years (133Mpc) from the Earth. It is one of the closest blazars to Earth, making it one of the brightest quasars in the night sky. It is suspected to have a supermassive black hole (SMBH) at its center due to its active nature, and has a companion galaxy (Markarian 421-5) that is fueling the gas jets observed pointing away from the galaxy.

Contents

It was first determined to be a very high energy gamma ray emitter in 1992 by M. Punch at the Whipple Observatory, and an extremely rapid outburst in very-high-energy gamma rays (15-minute rise-time) was measured in 1996 by J. Gaidos at Whipple Observatory

Markarian 421 also had an outburst in 2001 and is monitored by the Whole Earth Blazar Telescope project.

Due to its brightness (around 13.3 magnitude, max. 11.6 mag. and min. 16 mag.) the object can also be viewed by amateurs in smaller telescopes.

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References

Markarian 421 Wikipedia