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Emission nebula | |
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Planetary nebula | |
![]() As seen from Mount Lemmon Observatory | |
Observation data: J2000 epoch | |
Right ascension | 20h 31m 33.2s |
Declination | −07° 05′ 17″ |
Constellation | Aquila |
Notable features | A background galaxy gives it a "diamond ring" effect |
Designations | PK 038-25.1, PN G038.1-25.4 |
Abell 70 is a slightly elongated planetary nebula located 13,500-17,500 light years away in the constellation of Aquila. It is approaching the earth at 79 kilometers per second and expanding 38 kilometers per second. There is a galaxy named PMN J2033-0656 behind Abell 70, giving it a "diamond ring" effect.[1]
The faint OIII ring structure can be seen through a telescope.[2] The central star of Abell 70 is a binary star system consisting of a hot white dwarf and a G-type subgiant star.[3] The subgiant star is a barium star[1] that rotates rapidly (with a period of about 2 days) and is variable due to starspots.[3]
PMN J2033-0656 | |
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Observation data (J2000 epoch) | |
Right ascension | 20h 31m 33.1s[4] |
Declination | −07° 05′ 01″[4] |
Distance | 253 Mly (78 Mpc)[5] |
Characteristics | |
Apparent size (V) | 1.1' × 0.3'[4] |
Other designations | |
2MASX J20313312-0705014, 6dFGS gJ203133.1-070502, PGC 187663, LEDA 187663, NVSS J203133-070522[6] |
PMN J2033-0656 is an edge-on radio galaxy. Its position gives Abell 70 a diamond ring effect at its northern edge.[1]