SN 2026jkb

Summary

SN 2026jkb is a supernova^[1].

Key Facts

• SN 2026jkb is credited with the discovery of Gravitational-wave Optical Transient Observer^[2].
• SN 2026jkb's instance of is recorded as supernova^[3].
• SN 2026jkb's constellation is recorded as Centaurus^[4].
• SN 2026jkb's spectral class is recorded as SN.Ia^[5].
• SN 2026jkb's part of is recorded as Q1106397^[6].
• SN 2026jkb's time of discovery or invention is recorded as +2026-04-12T00:00:00Z^[7].
• SN 2026jkb's redshift is recorded as {'unit': '1', 'amount': '+0.0009'}^[8].
• SN 2026jkb's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.57'}^[9].
• SN 2026jkb's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+174.59121125'}^[10].
• SN 2026jkb's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-50.71853625'}^[11].
• SN 2026jkb's epoch is recorded as J2000.0^[12].

Body

Geography

SN 2026jkb's part of is recorded as Q1106397^[6].

Designation and Status

SN 2026jkb's instance of is recorded as supernova^[3].