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| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Eridanus [1] |
| Right ascension | 04h 16m 08.84s [2] |
| Declination | −24° 03′ 58.6″ [2] |
| Characteristics | |
| A | |
| Evolutionary stage | Blue supergiant [2] |
| B | |
| Evolutionary stage | Yellow hypergiant [2] |
| Astrometry | |
| Distance | 17.6 billion [2] ly |
| Details [2] | |
| A | |
| Luminosity | 125,000 L☉ |
| Temperature | 14,000 K |
| B | |
| Luminosity | 50,000 L☉ |
| Temperature | 5,250 K |
| Other designations | |
| EMO J041608.8-240358 [2] | |
Mothra, or EMO J041608.838-240358.60, is a binary system with a possible transient, [3] in the constellation of Eridanus. Mothra is in one of the strongly lensed galaxies behind the galaxy cluster MACS J0416.1-2403, nicknamed the "Christmas Tree Galaxy Cluster". [4]
The Mothra system is located at redshift z = 2.091 or about 10.5 billion light years away, and is notable for being one of the most distant star systems ever discovered. [2]
The Mothra system is located in is LS1. LS1 is believed to be 10,000-1,000,000 M☉ and is classified as a dwarf galaxy or globular cluster. LS1 and the Mothra system are behind the galaxy cluster MACS J0416.1-2403, and they used to same galaxy cluster as a gravitational lens to discover LS1 and Mothra. [5]
Mothra consists of two supergiant stars, a yellow supergiant/hypergiant? and a blue supergiant. As of 2025, the orbital characteristics of the Mothra system is unknown. [2]
The primary component of the Mothra system is classified as a yellow supergiant or yellow hypergiant.
Mothra A has a size of 271 R☉, a luminosity of 50,000 L☉, a temperature of 5,250 K, and has an initial mass of 15 M☉. [2]
The secondary component of the Mothra system is classified as a blue supergiant.
Mothra B has a size of 60 R☉, a luminosity of 125,000 L☉, and a temperature of 14,000 K. [5] [2]