This addon adds two hypothetical planetary systems around fast radio burst (FRB) sources - SGR 1935+2154, in the Milky Way, surrounded by the supernova remnant SNR G057.2+0.8 (also in this addon), and FRB 180916, located in the small spiral galaxy SDSS J015800.28+654253.0, located almost 500 million light years away in Cassiopeia. Two papers, authored by the same people, propose a planetary explanation for the fast radio bursts - the papers propose that they are created when a planet on an extremely eccentric orbit reaches periastron and is slightly disrupted, and the fragments that are ripped off the planet interact with the star, producing these bursts.
SGR 1935+2154's planet
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Paper - https://arxiv.org/abs/2403.13333 which also propses a system around SGR 1806-20, in the cluster Cl 1806-20.
Here is the link to the addon: viewtopic.php?p=163450#p163450
FRB 180916 and its planet in SDSS J015800.28+654253.0
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Paper - https://iopscience.iop.org/article/10.3847/1538-4357/ac558f (also proposes a system around FRB 121102, but since it's more than 2.5 Gly away, beyond the current 1 Gly render limit, I could not add it into Celestia)
Project Sisyphus - Texturing/painting every exoplanet known
- Trolligi 112477
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Tidal Disruption Systems
no more science papers
- Galaxy-Leaper
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Kepler-420
Kepler-420 is a binary star system, it takes 3430 ± 1200 days for these two stars to revolve around each other, and it is known that the host star A has a Jupiter-sized planet. It orbits its host star with a period of 86.647661 d ± 3 s and a high eccentricity of 0.772 ± 0.045.
viewtopic.php?p=163466#p163466
Kepler-420 is a binary star system, it takes 3430 ± 1200 days for these two stars to revolve around each other, and it is known that the host star A has a Jupiter-sized planet. It orbits its host star with a period of 86.647661 d ± 3 s and a high eccentricity of 0.772 ± 0.045.
viewtopic.php?p=163466#p163466
- Trolligi 112477
- Posts: 279
- Joined: 18.04.2020
- Age: 17
- With us: 4 years 10 months
- Location: London
GJ 1289
a nearby red dwarf with a sub-Neptune companion
GJ 1289's sole sub-Neptune
GJ 1289 is a red dwarf located about 27.28 lightyears from the solar system. A single sub-Neptune mass planet was detected around this star with an orbital period of 111.74 days.
[Download] (7.45 MB)
a nearby red dwarf with a sub-Neptune companion
GJ 1289's sole sub-Neptune
GJ 1289 is a red dwarf located about 27.28 lightyears from the solar system. A single sub-Neptune mass planet was detected around this star with an orbital period of 111.74 days.
[Download] (7.45 MB)
TOI-1468
a red dwarf with planets within their respective valleys
Both planets of TOI-1468
TOI-1468 is a red dwarf located about 80.63 light years from the solar system. Two planets are currently known to orbit this star, a high density super-Earth planet and an Oceanic sub-Neptune.
[Download] (2.87 MB)
Updated: TOI-1685
a red dwarf with planets within their respective valleys
Both planets of TOI-1468
TOI-1468 is a red dwarf located about 80.63 light years from the solar system. Two planets are currently known to orbit this star, a high density super-Earth planet and an Oceanic sub-Neptune.
[Download] (2.87 MB)
Updated: TOI-1685