In this article, the importance of NGC 6984 in today's society will be discussed. NGC 6984 has become a relevant topic in various areas, from politics to popular culture. Its influence extends globally, generating debates and reflections on its impact on our lives. Through detailed analysis, different perspectives and approaches on NGC 6984 will be explored, with the aim of understanding its true nature and meaning in the current context. Furthermore, the implications and consequences of NGC 6984 in the contemporary world will be examined, thus providing a complete overview of its relevance and significance.
NGC 6984 | |
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![]() NGC 6984 imaged by the Hubble Space Telescope | |
Observation data (J2000 epoch) | |
Constellation | Indus |
Right ascension | 20h 57m 53.987s[1] |
Declination | −51° 52′ 15.13″[1] |
Redshift | 0.015386[1] |
Heliocentric radial velocity | 4577 km/s[1] |
Distance | 180 million ly[2] |
Apparent magnitude (V) | 12.65[1] |
Apparent magnitude (B) | 13.19[1] |
Surface brightness | 22.82 mag/arcsec2[3] |
magnitude (J) | 10.94[3] |
magnitude (H) | 10.25[3] |
magnitude (K) | 9.99[3] |
Characteristics | |
Type | Spiral (SAc)[3] |
Apparent size (V) | 1.403 x 1.038 arcmin[1] |
Other designations | |
IRAS 20543-5203, 2MASX J20575398-5152151, PGC 65798, AM 2054-520, APMBGC 235+046+104, ISOSS J20578-5152, SGC 205419-5203.8, ESO 235- G 020 |
NGC 6984 is a barred spiral galaxy located 180 million light years away in the constellation Indus. It is a Type II Seyfert galaxy, a type of Active galactic nucleus (AGN).[4] It is situated south of the celestial equator, and is visible with the help of a telescope having an aperture of 10 inches (250 mm) or more.[3] It was discovered on 8 July 1834 by British astronomer John Herschel.[5]
NGC 6984 is notable for having been the host of two supernovae which occurred in the same location (< 0.4 arcsec),[6] about 1 year apart: SN 2012im (type Ic, mag. 18.9),[7] first known as SNhunt142,[8][9][10] and SN 2013ek (type Ib/c, mag. 16.9).[11][12] Hubble Space Telescope observations were initiated by Dr. Dan Milisavljevic.[13] NASA's press release about SN 2013ek said:
"It is so close to where SN 2012im was spotted that the two events are thought to be linked; the chance of two completely independent supernovae so close together and of the same class exploding within one year of one another is a very unlikely event. It was initially suggested that SN 2013ek may in fact be SN 2012im flaring up again, but further observations support the idea that they are separate supernovae — although they may be closely related in some as-yet-unknown way."[14]