![]() Hubble Space Telescope image of SN 1994D, visible at lower left | |
Event type | Supernova |
---|---|
Type Ia [1] | |
Date | c. 55.15 million years ago (discovered 7 March 1994 by R. Treffers) [2] |
Instrument | Leuschner Observatory |
Constellation | Virgo |
Right ascension | 12h 34m 02.395s [1] |
Declination | +07° 42′ 05.70″ [1] |
Epoch | B2000.0 |
Distance | ~55.15 million ly |
Redshift | 0.0036, 0.0001, −0.0001, 0.0021, 0.0023, 0.0022, 0.0008, 0.0005, 0.0013, 0.0017, 0.0004, 0.0024, 0.0011, 0.0012, 0.0002 |
Host | NGC 4526 [2] |
Progenitor type | White dwarf |
Peak apparent magnitude | +11.9 [3] |
Other designations | SN 1994D, AAVSO 1229+08 |
Preceded by | SN 1994C [4] |
Followed by | SN 1994E [4] |
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SN 1994D was a Type Ia supernova event in the outskirts of galaxy NGC 4526, which was observed in 1994.
It was offset by 9.0″ west and 7.8″ south of the galaxy center and positioned near a prominent dust lane. [1] It was caused by the explosion of a white dwarf star composed of carbon and oxygen. [5] This event was discovered on March 7, 1994 by R. R. Treffers and associates using the automated 30-inch telescope at Leuschner Observatory. [2] It reached peak visual brightness, magnitude 11.9, two weeks later on March 22. [5] [3] Modelling of the light curve indicates the explosion would have been visible around March 3-4. A possible detection of helium in the spectrum was made by W. P. S. Meikle and associates in 1996. [1] A mass of 0.014 to 0.03 M☉ in helium would be needed to produce this feature. [6]