Project Sisyphus - Texturing/painting every exoplanet known
- SevenSpheres
- Moderator
- Posts: 822
- Joined: 08.10.2019
- With us: 4 years 10 months
Kepler-138
Low-mass, low-density worlds
Kepler-138, also known as KOI-314, is a red dwarf star about 219 light-years away in the constellation Lyra, which hosts four known planets. Kepler-138 c & d are both about 1.5 times the size of Earth; they were originally estimated to have very different masses and densities, but were found in 2022 to be similarly low-density, volatile-rich "ocean worlds". Kepler-138 b is the second-least massive exoplanet with a measured mass (after Draugr), between that of Mars and Mercury, and also has a low density, though it's certainly rocky given how small it is. Kepler-138 e is almost half the mass of Earth; it was discovered through transit timing variations of the other planets, and is the least massive exoplanet found by this method.
The textures for the star and planet b, and the surface texture for planet e, have been taken from the addon for this system by adios.
Kepler-22 & 62
Kepler's first habitable zone planets
Kepler-22 b, Kepler-62 e, and Kepler-62 f were the first planets in the habitable zone discovered by the Kepler mission. In particular, Kepler-62 f (announced 10 years ago this month) is small enough that it most likely has a rocky composition, and can be considered the first good candidate for a potentially habitable exoplanet. On the other hand, Kepler-22 b is just over twice the size of Earth, and it was realized even at the time of discovery that it was unlikely to have a rocky composition, which has recently been confirmed by upper limits on its mass. Instead, it's somewhere on the "ocean world" to "mini-Neptune" continuum.
This version of Kepler-22 b was originally included in my old "Exoplanet Updates" addon in 2019, and a modified version of it was released by fyr02 in 2020 here ("Vaporian"). I've just re-released it with updated data.
There's already a good addon for Kepler-62 by MrSpace43 here, with textures based on the NASA artistic impressions. My addon only includes textures for Kepler-62 f. The default texture is the "official" NASA one, from the same (now gone?) source as MrSpace43's Kepler-22 b and my Kepler-186 f, and the alternate surface shows the planet covered by an ocean.
Might as well attach my Kepler-452 b addon here as well, since it didn't have a dedicated post, having been part of "Exoplanet Updates" and then just submitted to celestia.mobi. This is another habitable zone planet, though again fairly large and technically a planet candidate. It's just using the NASA texture, unmodified.
Low-mass, low-density worlds
Kepler-138, also known as KOI-314, is a red dwarf star about 219 light-years away in the constellation Lyra, which hosts four known planets. Kepler-138 c & d are both about 1.5 times the size of Earth; they were originally estimated to have very different masses and densities, but were found in 2022 to be similarly low-density, volatile-rich "ocean worlds". Kepler-138 b is the second-least massive exoplanet with a measured mass (after Draugr), between that of Mars and Mercury, and also has a low density, though it's certainly rocky given how small it is. Kepler-138 e is almost half the mass of Earth; it was discovered through transit timing variations of the other planets, and is the least massive exoplanet found by this method.
The textures for the star and planet b, and the surface texture for planet e, have been taken from the addon for this system by adios.
Kepler-22 & 62
Kepler's first habitable zone planets
Kepler-22 b, Kepler-62 e, and Kepler-62 f were the first planets in the habitable zone discovered by the Kepler mission. In particular, Kepler-62 f (announced 10 years ago this month) is small enough that it most likely has a rocky composition, and can be considered the first good candidate for a potentially habitable exoplanet. On the other hand, Kepler-22 b is just over twice the size of Earth, and it was realized even at the time of discovery that it was unlikely to have a rocky composition, which has recently been confirmed by upper limits on its mass. Instead, it's somewhere on the "ocean world" to "mini-Neptune" continuum.
This version of Kepler-22 b was originally included in my old "Exoplanet Updates" addon in 2019, and a modified version of it was released by fyr02 in 2020 here ("Vaporian"). I've just re-released it with updated data.
There's already a good addon for Kepler-62 by MrSpace43 here, with textures based on the NASA artistic impressions. My addon only includes textures for Kepler-62 f. The default texture is the "official" NASA one, from the same (now gone?) source as MrSpace43's Kepler-22 b and my Kepler-186 f, and the alternate surface shows the planet covered by an ocean.
Might as well attach my Kepler-452 b addon here as well, since it didn't have a dedicated post, having been part of "Exoplanet Updates" and then just submitted to celestia.mobi. This is another habitable zone planet, though again fairly large and technically a planet candidate. It's just using the NASA texture, unmodified.
My Addons: viewtopic.php?f=23&t=19978 • Discord server admin
Celestia versions: 1.5.1, 1.6.1, 1.6.2, 1.7.0, and some unofficial versions like Celestia-ED
Celestia versions: 1.5.1, 1.6.1, 1.6.2, 1.7.0, and some unofficial versions like Celestia-ED
- SevenSpheres
- Moderator
- Posts: 822
- Joined: 08.10.2019
- With us: 4 years 10 months
GJ 1214
Orkaria & Enaiposha
GJ 1214 is a red dwarf star 47.8 light-years away in the constellation Ophiuchus. Its one known planet was the second super-Earth/sub-Neptune observed to transit its host star. The planet has a low density, indicating a volatile-rich composition, and recent observations by JWST reveal a hazy, reflective atmosphere mainly composed of water vapor or methane, without significant amounts of hydrogen.
This addon includes a fictional texture for GJ 1214 b depicting its hazy appearance, as well as an older texture by Edasich from 2010 and a temperature map from the Kempton et al. 2023 paper. The reprojected temperature map isn't perfect and could use improvement!
Minor update 2023-06-08 after NameExoWorlds results were announced.
Orkaria & Enaiposha
GJ 1214 is a red dwarf star 47.8 light-years away in the constellation Ophiuchus. Its one known planet was the second super-Earth/sub-Neptune observed to transit its host star. The planet has a low density, indicating a volatile-rich composition, and recent observations by JWST reveal a hazy, reflective atmosphere mainly composed of water vapor or methane, without significant amounts of hydrogen.
This addon includes a fictional texture for GJ 1214 b depicting its hazy appearance, as well as an older texture by Edasich from 2010 and a temperature map from the Kempton et al. 2023 paper. The reprojected temperature map isn't perfect and could use improvement!
Minor update 2023-06-08 after NameExoWorlds results were announced.
My Addons: viewtopic.php?f=23&t=19978 • Discord server admin
Celestia versions: 1.5.1, 1.6.1, 1.6.2, 1.7.0, and some unofficial versions like Celestia-ED
Celestia versions: 1.5.1, 1.6.1, 1.6.2, 1.7.0, and some unofficial versions like Celestia-ED
TOI-540
a nearby system with a barren rocky world
the stripped rocky world that is TOI-540 b
TOI-540 is a red dwarf located about 45.64 light-years away from the solar system. The star has a single Sub-Earth (b= 0.90 Re) rocky planet orbiting it. The star itself has a high X-ray emission which would cause the planet orbiting it to undergo severe atmosphere erosion, additionally, due to its somewhat close proximity to the solar system, it could be a target for transmission and emission spectroscopy with JWST
Also, welcome back, I'm gonna explain what's gonna go down regarding everything that I've done. I've made around 40 add-ons since the forum went down back in April and now since it's back online they all gotta be dumped here. So every day (or so) im gonna post one new stellar system addon and one remake of a previous stellar system (with some exceptions, like this post).
a nearby system with a barren rocky world
the stripped rocky world that is TOI-540 b
TOI-540 is a red dwarf located about 45.64 light-years away from the solar system. The star has a single Sub-Earth (b= 0.90 Re) rocky planet orbiting it. The star itself has a high X-ray emission which would cause the planet orbiting it to undergo severe atmosphere erosion, additionally, due to its somewhat close proximity to the solar system, it could be a target for transmission and emission spectroscopy with JWST
Also, welcome back, I'm gonna explain what's gonna go down regarding everything that I've done. I've made around 40 add-ons since the forum went down back in April and now since it's back online they all gotta be dumped here. So every day (or so) im gonna post one new stellar system addon and one remake of a previous stellar system (with some exceptions, like this post).
TOI-2095
a diplanetary system of two potentially Venus-like planets
Both super-Earths of TOI-2095
TOI-2095 is an M-type main sequence star located about 136.72 lightyears from the solar system. Two potentially Venus-like super-Earths (b= 1.25 Re | c= 1.32 Re) are hosted by the star, with TOI-2095 c orbiting very close to the habitable zone. the masses of these planets haven't been accurately determined so only upper limits have been placed (b < 4.1 Me | c < 7.4 Me)
The remake bundled with this is a system less than a hundred lightyears away from the one listed above: TOI-2096
a diplanetary system of two potentially Venus-like planets
Both super-Earths of TOI-2095
TOI-2095 is an M-type main sequence star located about 136.72 lightyears from the solar system. Two potentially Venus-like super-Earths (b= 1.25 Re | c= 1.32 Re) are hosted by the star, with TOI-2095 c orbiting very close to the habitable zone. the masses of these planets haven't been accurately determined so only upper limits have been placed (b < 4.1 Me | c < 7.4 Me)
The remake bundled with this is a system less than a hundred lightyears away from the one listed above: TOI-2096
Hot Jupiter TOIs
A collection of eight TOI hot Jupiter systems
All eight hot Jupiters
This one is a large addon pack, containing 8 systems of hot Jupiters. the eight that are featured are (in order): TOI-2818, TOI-1811, TOI-2145, TOI-2152, TOI-2583, TOI-2587, TOI-2796, and TOI-2803. Several of these are in binary systems with one being in a trinary system, one has an interior super-Earth candidate (though not included within this addon pack) and at least one orbits a sub-giant star.
The file below contains the zip files for all of the hot Jupiters, so if you only want some of them you can just grab the from the main zip and delete the rest. I decided this would be more efficient than flooding the thread with a bunch of single-planet systems, especially since they are all so similar to each other.
the remakes for this are also hot Jupiters: TOI-1937 and TOI-2364
A collection of eight TOI hot Jupiter systems
All eight hot Jupiters
This one is a large addon pack, containing 8 systems of hot Jupiters. the eight that are featured are (in order): TOI-2818, TOI-1811, TOI-2145, TOI-2152, TOI-2583, TOI-2587, TOI-2796, and TOI-2803. Several of these are in binary systems with one being in a trinary system, one has an interior super-Earth candidate (though not included within this addon pack) and at least one orbits a sub-giant star.
The file below contains the zip files for all of the hot Jupiters, so if you only want some of them you can just grab the from the main zip and delete the rest. I decided this would be more efficient than flooding the thread with a bunch of single-planet systems, especially since they are all so similar to each other.
the remakes for this are also hot Jupiters: TOI-1937 and TOI-2364
TOI-2000
a diplanetary system of a hot Jupiter with an interior hot mini-Neptune
both hot worlds of TOI-2000
TOI-2000 is a metal-rich ([Fe/H] = 0.439) G-type star located about 566.2 lightyears from the solar system. The star has two hot gaseous planets, a dense mini-Neptune (b= 2.7 Re, 11 Me) and a Saturn-like planet (c= 8.14 Re, 81.7 Me). The system is optimal for the study of the formation of hot Jupiters due to the existence of the innermost planet
Remake:
TOI-237
a red dwarf home to a possibly Venus-like super-Earth
TOI-237 b depicted as a super-Venus
TOI-237 is a red dwarf located about 124.31 lightyears from the solar system. The star hosts a single potentially Venus-like super-Earth planet (b= 1.44 Re). Astronauta/Betegelge originally made this addon, their original texture for the planet's surface is included as an alternate surface within the addon files
a diplanetary system of a hot Jupiter with an interior hot mini-Neptune
both hot worlds of TOI-2000
TOI-2000 is a metal-rich ([Fe/H] = 0.439) G-type star located about 566.2 lightyears from the solar system. The star has two hot gaseous planets, a dense mini-Neptune (b= 2.7 Re, 11 Me) and a Saturn-like planet (c= 8.14 Re, 81.7 Me). The system is optimal for the study of the formation of hot Jupiters due to the existence of the innermost planet
Remake:
TOI-237
a red dwarf home to a possibly Venus-like super-Earth
TOI-237 b depicted as a super-Venus
TOI-237 is a red dwarf located about 124.31 lightyears from the solar system. The star hosts a single potentially Venus-like super-Earth planet (b= 1.44 Re). Astronauta/Betegelge originally made this addon, their original texture for the planet's surface is included as an alternate surface within the addon files
TOI-2076
a compact little Neptune system
all three Neptune like planets orbiting TOI-2076
TOI-2076 is a K-type star located about 136.59 lightyears from the solar system. The star has 3 warm Neptune-like planets orbiting within 0.2 AU (b= 2.518 Re, c= 3.497 Re, 3.232 Re). planets b and c exhibit TTVs and are near a 2:1 MMR, However, the model of said TTVs was not accurate enough to derive planet masses, and with no RV measurements, none of the planet's accurate masses are known.
Remake:
TOI-1807
A super-Earth possibly covered with lava
The molten world that is TOI-1807 b with the Triangulum Galaxy
TOI-1807 is a K-type star located about 139.04 lightyears from the solar system. A single hot super-Earth (b= 1.37 Re, 2.57 Me) orbits this star every 13.19 hours. This is a remake of an addon originally made by SolHorizon, their original texture is included as an alt surface for the planet.
a compact little Neptune system
all three Neptune like planets orbiting TOI-2076
TOI-2076 is a K-type star located about 136.59 lightyears from the solar system. The star has 3 warm Neptune-like planets orbiting within 0.2 AU (b= 2.518 Re, c= 3.497 Re, 3.232 Re). planets b and c exhibit TTVs and are near a 2:1 MMR, However, the model of said TTVs was not accurate enough to derive planet masses, and with no RV measurements, none of the planet's accurate masses are known.
Remake:
TOI-1807
A super-Earth possibly covered with lava
The molten world that is TOI-1807 b with the Triangulum Galaxy
TOI-1807 is a K-type star located about 139.04 lightyears from the solar system. A single hot super-Earth (b= 1.37 Re, 2.57 Me) orbits this star every 13.19 hours. This is a remake of an addon originally made by SolHorizon, their original texture is included as an alt surface for the planet.
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Topic authorGurren Lagann
- Posts: 433
- Joined: 31.01.2018
- Age: 18
- With us: 6 years 7 months
- Location: State of Rio de Janeiro, Brazil
KMT-2016-BLG-1397L
Seventeen time!
LOri167
LOring in wide youth
Upper Scorpius Rogue Planets
Solitude in Upper S
July 3rd again... Forums are back so here are 3 addons to Sisyphy my birthday!
Seventeen time!
LOri167
LOring in wide youth
Upper Scorpius Rogue Planets
Solitude in Upper S
July 3rd again... Forums are back so here are 3 addons to Sisyphy my birthday!
"The tomorrow we're trying to reach is not a tomorrow you had decided on!"
- Simon the Digger
"Nothing is impossible for me, as long I'm determinated to keep moving forward!"
"If other people aren't going to do it, I'm going to do it myself!"
- Me (Gurren)
Current major projects:
- Aur Cir
- Cel+
- Project Sisyphus
- Populating the Local Group
- An galaxy generator
- Simon the Digger
"Nothing is impossible for me, as long I'm determinated to keep moving forward!"
"If other people aren't going to do it, I'm going to do it myself!"
- Me (Gurren)
Current major projects:
- Aur Cir
- Cel+
- Project Sisyphus
- Populating the Local Group
- An galaxy generator
-
- Posts: 196
- Joined: 21.10.2021
- Age: 16
- With us: 2 years 10 months
- Location: Novo Hamburgo, State of Rio Grande do Sul, Brazil
Update CFBDSIR 2149-0403: viewtopic.php?p=158741#p158741
TOI-969
A diplanetary system of a hot mini-Neptune and a cold super-Jupiter
The distant planets of TOI-969
TOI-969 is a K-type main-sequence star located about 251.87 lightyears from the solar system, the star has two planets: a transiting hot mini-Neptune (b= 2.765 Re, 9.10 Me) and a non-transiting super-Jupiter (c= 11.3 Mj). The system is unique for having two gaseous planets at wildly different temperatures with TOI-969 b predicted to be around 10x hotter than TOI-969 c.
Remake: TOI-2257
A diplanetary system of a hot mini-Neptune and a cold super-Jupiter
The distant planets of TOI-969
TOI-969 is a K-type main-sequence star located about 251.87 lightyears from the solar system, the star has two planets: a transiting hot mini-Neptune (b= 2.765 Re, 9.10 Me) and a non-transiting super-Jupiter (c= 11.3 Mj). The system is unique for having two gaseous planets at wildly different temperatures with TOI-969 b predicted to be around 10x hotter than TOI-969 c.
Remake: TOI-2257
TOI-1266
Two maybe three mini-Neptunes in a compact system
Both worlds of TOI-1266
TOI-1266 is an M-type dwarf star located about 117.39 lightyears from the solar system. The star hosts two planets: a warm mini-Neptune, and a slightly cooler oceanic planet. Both planets likely have large envelopes with planet c being more volatile rich. There is additional evidence suggesting another planet with a similar mass to the inner most planet orbits on the boundary of TOI-1266's habitable zone.
TOI-1266's candidate planet
[Download Confirmed] (7.09 MB)
[Download Unconfirmed] (3.09 MB)
Remake: HD 23472
Two maybe three mini-Neptunes in a compact system
Both worlds of TOI-1266
TOI-1266 is an M-type dwarf star located about 117.39 lightyears from the solar system. The star hosts two planets: a warm mini-Neptune, and a slightly cooler oceanic planet. Both planets likely have large envelopes with planet c being more volatile rich. There is additional evidence suggesting another planet with a similar mass to the inner most planet orbits on the boundary of TOI-1266's habitable zone.
TOI-1266's candidate planet
[Download Confirmed] (7.09 MB)
[Download Unconfirmed] (3.09 MB)
Remake: HD 23472
Last edited by Karistus_ on 24.11.2023, 05:59, edited 1 time in total.
TOI-715
a large potentially rocky world within the habitable zone
TOI-715 b depicted as a rocky, Earth-like planet
TOI-715 b depicted as a water-world
TOI-715 is a red dwarf located about 138.42 lightyears from the solar system. A single potentially rocky super-Earth (b= 1.55 Re) orbits well within the star's habitable zone, no mass measurements of this planet have been taken yet.
There is an additional planet candidate within the system, TOI-715.02 (TIC 271971130.02), which is predicted to be around the same size as Earth (.02= 1.066 Re) and is also predicted to orbit within the outer boundary of TOI-715's habitable zone
If this planet is confirmed, it would make it one of the smallest planets found with the (conservative) habitable zone discovered by TESS
The second candidate planet of TOI-715
confirmed planet
candidate planet
Remake: Kepler-174
a large potentially rocky world within the habitable zone
TOI-715 b depicted as a rocky, Earth-like planet
TOI-715 b depicted as a water-world
TOI-715 is a red dwarf located about 138.42 lightyears from the solar system. A single potentially rocky super-Earth (b= 1.55 Re) orbits well within the star's habitable zone, no mass measurements of this planet have been taken yet.
There is an additional planet candidate within the system, TOI-715.02 (TIC 271971130.02), which is predicted to be around the same size as Earth (.02= 1.066 Re) and is also predicted to orbit within the outer boundary of TOI-715's habitable zone
If this planet is confirmed, it would make it one of the smallest planets found with the (conservative) habitable zone discovered by TESS
The second candidate planet of TOI-715
confirmed planet
candidate planet
Remake: Kepler-174
TOI-2445
a red dwarf with a short period super-Earth
the near-molten world that is TOI-2445 b
TOI-2445 is a red dwarf located about 158.38 lightyears from the solar system, a single larger-than-earth planet (b= 1.25 Re) orbits close to its host. The planet's mass hasn't been fully analyzed, so only upper limits have been placed (b= <18 Me).
Remake:
TOI-2109
a Jupiter-sized planet hotter than some stars
TOI-2109 b and its host
TOI-2109 is an F-type star located about 854.25 lightyears from the solar system. The star has a single hot gas giant that's larger (b= 1.35 Rj) and more massive (b= 5.02 Mj) than Jupiter. The planet completes an orbit every 16 hours and is scorching, with an estimated temperature of 3646 Kelvin, making it hotter than some red dwarf stars.
This is a remake of the addon made by SolHorizon. Their original textures are included in the zip file
a red dwarf with a short period super-Earth
the near-molten world that is TOI-2445 b
TOI-2445 is a red dwarf located about 158.38 lightyears from the solar system, a single larger-than-earth planet (b= 1.25 Re) orbits close to its host. The planet's mass hasn't been fully analyzed, so only upper limits have been placed (b= <18 Me).
Remake:
TOI-2109
a Jupiter-sized planet hotter than some stars
TOI-2109 b and its host
TOI-2109 is an F-type star located about 854.25 lightyears from the solar system. The star has a single hot gas giant that's larger (b= 1.35 Rj) and more massive (b= 5.02 Mj) than Jupiter. The planet completes an orbit every 16 hours and is scorching, with an estimated temperature of 3646 Kelvin, making it hotter than some red dwarf stars.
This is a remake of the addon made by SolHorizon. Their original textures are included in the zip file
TOI-216
a diplanetary system with a puffy sub-Jupiter
Both gaseous worlds of TOI-216
TOI-216 is a K-type main sequence star located about 580.12 lightyears from the solar system. Two warm sub-Jupiter planets orbit this star in a 2:1 MMR (b= 7.28 Re, 17.6 Me | c= 10.08 Re, 166.85 Me). TOI-216 b has a low density and has been revealed to be very puffy.
Remake:
Kepler-443
a lone temperate mini-Neptune
the isolated world of Kepler-443
Kepler-443, aka KOI-4745, is a K-type dwarf star located about 2,677 lightyears from the solar system. A single mini-Neptune (b= 2.35 Re) orbits within the star's habitable zone, the mass of this planet is unknown currently.
This add-on was initially made by SolHorizon, who depicted the planet as Earth-like. But with this update, the original textures have been removed. though the original texture is still present here
a diplanetary system with a puffy sub-Jupiter
Both gaseous worlds of TOI-216
TOI-216 is a K-type main sequence star located about 580.12 lightyears from the solar system. Two warm sub-Jupiter planets orbit this star in a 2:1 MMR (b= 7.28 Re, 17.6 Me | c= 10.08 Re, 166.85 Me). TOI-216 b has a low density and has been revealed to be very puffy.
Remake:
Kepler-443
a lone temperate mini-Neptune
the isolated world of Kepler-443
Kepler-443, aka KOI-4745, is a K-type dwarf star located about 2,677 lightyears from the solar system. A single mini-Neptune (b= 2.35 Re) orbits within the star's habitable zone, the mass of this planet is unknown currently.
This add-on was initially made by SolHorizon, who depicted the planet as Earth-like. But with this update, the original textures have been removed. though the original texture is still present here
Kepler-1181
a diplanetary system of two hot super-Earths
both ultra hot worlds of Kepler-1181
Kepler-1181, aka KOI-2303, is an F-type main sequence star located about 3059.25 lightyears from the solar system. two hot super-Earths (b= 1.59 Re, c= 1.74 Re) orbit this star at a distance no greater than 0.093 AU.
Remake:
Kepler-283
a system with a warm mini-Neptune and a temperate one
both mini-Neptunes of Kepler-283. Kepler-283 c is depicted as an ocean world
Kepler-283, aka KOI-1298, is a K-type main sequence star located about 1,525.97 light years from the solar system. The star hosts two mini-Neptunes (b= 2.371 Re, c= 2.055 Re), the outermost orbits within the host's habitable zone. There are no mass measurements of any of these planets
The original addon was made by SolHorizon and Jon van Vilet. both textures have been included as alt surfaces to the new ones
a diplanetary system of two hot super-Earths
both ultra hot worlds of Kepler-1181
Kepler-1181, aka KOI-2303, is an F-type main sequence star located about 3059.25 lightyears from the solar system. two hot super-Earths (b= 1.59 Re, c= 1.74 Re) orbit this star at a distance no greater than 0.093 AU.
Remake:
Kepler-283
a system with a warm mini-Neptune and a temperate one
both mini-Neptunes of Kepler-283. Kepler-283 c is depicted as an ocean world
Kepler-283, aka KOI-1298, is a K-type main sequence star located about 1,525.97 light years from the solar system. The star hosts two mini-Neptunes (b= 2.371 Re, c= 2.055 Re), the outermost orbits within the host's habitable zone. There are no mass measurements of any of these planets
The original addon was made by SolHorizon and Jon van Vilet. both textures have been included as alt surfaces to the new ones
TOI-4010
three hot-to-warm gaseous planets joined by a Jupiter-like planet
all planets of TOI-4010
TOI-4010 is a metal-rich ([Fe/H] = 0.37) K-type main-sequence star located about 578.94 light years from the solar system. 4 gaseous planets orbit this star (b= 3.02 Re, 11 Me | c= 5.93 Re, 20.31 Me | d= 6.18 Re, 38.15 Me | e= 692 Me). The inner two planets (planets b and c) are near a 4:1 MMR but don't show any significant TTVs, additionally, the study that confirmed the system's existence stated that they don't know whether TOI-4010 e doesn't transit or just hasn't had any of its possible transits recorded
Remake: TOI-451
three hot-to-warm gaseous planets joined by a Jupiter-like planet
all planets of TOI-4010
TOI-4010 is a metal-rich ([Fe/H] = 0.37) K-type main-sequence star located about 578.94 light years from the solar system. 4 gaseous planets orbit this star (b= 3.02 Re, 11 Me | c= 5.93 Re, 20.31 Me | d= 6.18 Re, 38.15 Me | e= 692 Me). The inner two planets (planets b and c) are near a 4:1 MMR but don't show any significant TTVs, additionally, the study that confirmed the system's existence stated that they don't know whether TOI-4010 e doesn't transit or just hasn't had any of its possible transits recorded
Remake: TOI-451
HD 56414 and TOI-824
two ultra-hot Neptunes
The Neptune-class planet that is HD 56414 b
HD 56414 is an A-type main sequence star located about 887.43 lightyears from the solar system, the star has a single hot Neptune-sized planet on a month-long orbit, its mass is currently unknown (b= 3.71 Re).
the boiling world that is TOI-824 b
TOI-824 is a K-type main sequence star located about 208.37 lightyears from the solar system. orbiting this star is a single, hot oceanic planet that completes a full orbit every 1.39 days (b= 2.926 Re, 18.467 Me). observations from Spitzer showed that planet had poor heat distribution and likely lacked a hydrogen dominated envelope and was either: a super-Earth with a volatile rich, extended atmosphere or a bare ocean world with a relatively thin atmosphere. Further JWST analysis could constrain where this planet falls into far greater than Spitzer could.
I figured I would put both of these objects in one post since they are similar to each other and I felt it was a waste to have them in separate posts. Each has an independent download.
[Download TOI-824] (569.64 KB)
Remake: TOI-712
two ultra-hot Neptunes
The Neptune-class planet that is HD 56414 b
HD 56414 is an A-type main sequence star located about 887.43 lightyears from the solar system, the star has a single hot Neptune-sized planet on a month-long orbit, its mass is currently unknown (b= 3.71 Re).
the boiling world that is TOI-824 b
TOI-824 is a K-type main sequence star located about 208.37 lightyears from the solar system. orbiting this star is a single, hot oceanic planet that completes a full orbit every 1.39 days (b= 2.926 Re, 18.467 Me). observations from Spitzer showed that planet had poor heat distribution and likely lacked a hydrogen dominated envelope and was either: a super-Earth with a volatile rich, extended atmosphere or a bare ocean world with a relatively thin atmosphere. Further JWST analysis could constrain where this planet falls into far greater than Spitzer could.
I figured I would put both of these objects in one post since they are similar to each other and I felt it was a waste to have them in separate posts. Each has an independent download.
[Download TOI-824] (569.64 KB)
Remake: TOI-712
Last edited by Karistus_ on 06.08.2023, 09:21, edited 1 time in total.
TOI-2525
a diplanetary system with a ..puffy sub-Jupiter ..huh
Both planets of TOI-2525
TOI-2525 is a K-type main sequence star located about 1289 lightyears from the solar system. The star has two warm sub-Jupiters close to a 2:1 MMR (b= 8.68 Re, 27 Me | c= 10.1 Re, 209 Me). The innermost planet has an extremely low density and is likely to be a puffy gas giant.
Remake: TOI-2285
a diplanetary system with a ..puffy sub-Jupiter ..huh
Both planets of TOI-2525
TOI-2525 is a K-type main sequence star located about 1289 lightyears from the solar system. The star has two warm sub-Jupiters close to a 2:1 MMR (b= 8.68 Re, 27 Me | c= 10.1 Re, 209 Me). The innermost planet has an extremely low density and is likely to be a puffy gas giant.
Remake: TOI-2285
GJ 9224
a hot super-Earth accompanied by three outer planets
all four planets hosted by GJ 9224
GJ 9224, also known as TOI-500, is a K-type star located about 154.49 lightyears away from the solar system. 4 planets, a molten Venus-like planet (b= 1.17 Re, 1.42 Me) and 3 Neptunian planets (c= 5.03 Me, d=33.12 Me, e= 15.05 Me) orbit the star interior to its HZ. The last three planets don't transit the star from our perspective, only the first one does and so we don't know their actual sizes.
Remake: GJ 1252
a hot super-Earth accompanied by three outer planets
all four planets hosted by GJ 9224
GJ 9224, also known as TOI-500, is a K-type star located about 154.49 lightyears away from the solar system. 4 planets, a molten Venus-like planet (b= 1.17 Re, 1.42 Me) and 3 Neptunian planets (c= 5.03 Me, d=33.12 Me, e= 15.05 Me) orbit the star interior to its HZ. The last three planets don't transit the star from our perspective, only the first one does and so we don't know their actual sizes.
Remake: GJ 1252
TOI-1685
a hot ocean world with a candidate mini-Neptune
the hot ocean world that is TOI-1685 b, which is also a target of study for JWST
TOI-1685 is an M-type main sequence star located about 122.64 light-years from the solar system. a single planet was confirmed around this star, a hot Ocean world which is a future target of study for James Webb (b= 1.7 Re, 3.78 Me).
Additionally, the study confirming TOI-1685 b (as an Ocean world) speaks of a second planet candidate, a possible mini-Neptune orbiting at 9.03 days (c= 9.21 Me), though they stated that they could not confidently confirm it as a planet due to the proposed orbit being close to the first harmonic of it's hosts rotational period
the second planet candidate of TOI-1685
[Download Confirmed Planet] (3.84 MB)
[Download Unconfirmed Planet] (0.92 MB)
Remake: TOI-1136
Added after 11 hours 40 minutes:
HD 108236
a sun-like star hosting 5 planets
all five sub-Neptunes of HD 108236
HD 108236, aka TOI-1233, is a metal-poor Sun-like star located about 210.6 lightyears from the solar system, the star hosts five planets: a super-Earth (b= 1.615 Re) and four mini-Neptunes (c= 2.071 Re | d= 2.539 Re | e= 3.083 Re | f= 2.017 Re) all of which orbit interior to the stars habitable zone. None of their masses are known.
Remake: TOI-1246
a hot ocean world with a candidate mini-Neptune
the hot ocean world that is TOI-1685 b, which is also a target of study for JWST
TOI-1685 is an M-type main sequence star located about 122.64 light-years from the solar system. a single planet was confirmed around this star, a hot Ocean world which is a future target of study for James Webb (b= 1.7 Re, 3.78 Me).
Additionally, the study confirming TOI-1685 b (as an Ocean world) speaks of a second planet candidate, a possible mini-Neptune orbiting at 9.03 days (c= 9.21 Me), though they stated that they could not confidently confirm it as a planet due to the proposed orbit being close to the first harmonic of it's hosts rotational period
the second planet candidate of TOI-1685
[Download Confirmed Planet] (3.84 MB)
[Download Unconfirmed Planet] (0.92 MB)
Remake: TOI-1136
Added after 11 hours 40 minutes:
HD 108236
a sun-like star hosting 5 planets
all five sub-Neptunes of HD 108236
HD 108236, aka TOI-1233, is a metal-poor Sun-like star located about 210.6 lightyears from the solar system, the star hosts five planets: a super-Earth (b= 1.615 Re) and four mini-Neptunes (c= 2.071 Re | d= 2.539 Re | e= 3.083 Re | f= 2.017 Re) all of which orbit interior to the stars habitable zone. None of their masses are known.
Remake: TOI-1246
Last edited by Karistus_ on 30.08.2023, 21:47, edited 1 time in total.