Project Sisyphus - Texturing/painting every exoplanet known
- DaveBowman2001
- Posts: 772
- Joined: 06.07.2018
- Age: 24
- With us: 6 years 1 month
- Location: Manila, Philippines
Kepler-1130
Two (or Four) Molten Sub-Earths Closer than Mercury's Orbit
Kepler-1130, also known as KOI-2169, is a binary star system of a K-type main sequence star and a red dwarf about 819 light-years away in the constellation Lyra. As of 2023, the larger star has two confirmed planets, with another two awaiting confirmation. All of them are smaller than Earth and are less than 8.5 million km from their star, indicating that all of their surfaces were molten
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Feb-19
Original link: https://pan.baidu.com/s/1WX4qhpUdv0tIEcAPe-Bdyg
Two (or Four) Molten Sub-Earths Closer than Mercury's Orbit
Kepler-1130, also known as KOI-2169, is a binary star system of a K-type main sequence star and a red dwarf about 819 light-years away in the constellation Lyra. As of 2023, the larger star has two confirmed planets, with another two awaiting confirmation. All of them are smaller than Earth and are less than 8.5 million km from their star, indicating that all of their surfaces were molten
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Feb-19
Original link: https://pan.baidu.com/s/1WX4qhpUdv0tIEcAPe-Bdyg
"Open the pod-bay doors HAL"
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
- DaveBowman2001
- Posts: 772
- Joined: 06.07.2018
- Age: 24
- With us: 6 years 1 month
- Location: Manila, Philippines
Kepler-199
Two Neptunes with Years Lasting a Month or Two
Kepler-199, also known as KOI-638, is a large Sun-like star about 1,725 light-years away in the constellation Cygnus. Two Neptune-sized planets were found occupying orbits lasting between 23 and 67 days respectively
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Feb-19
Original link: https://pan.baidu.com/s/1WX4qhpUdv0tIEcAPe-Bdyg
Two Neptunes with Years Lasting a Month or Two
Kepler-199, also known as KOI-638, is a large Sun-like star about 1,725 light-years away in the constellation Cygnus. Two Neptune-sized planets were found occupying orbits lasting between 23 and 67 days respectively
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Feb-19
Original link: https://pan.baidu.com/s/1WX4qhpUdv0tIEcAPe-Bdyg
"Open the pod-bay doors HAL"
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
- DaveBowman2001
- Posts: 772
- Joined: 06.07.2018
- Age: 24
- With us: 6 years 1 month
- Location: Manila, Philippines
WASP-28
A Scorching Hot Jupiter Twice the Heat of Venus
WASP-28, also known as K2-1 and TOI-4518, is an F-type main sequence star about 1,148 light-years away in the constellation Pisces. A gas giant larger than Jupiter but only 91% of its mass completes a 3.4-day orbit at only 6.5 million km from its parent star
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Feb-19
Original link: https://pan.baidu.com/s/1WX4qhpUdv0tIEcAPe-Bdyg
A Scorching Hot Jupiter Twice the Heat of Venus
WASP-28, also known as K2-1 and TOI-4518, is an F-type main sequence star about 1,148 light-years away in the constellation Pisces. A gas giant larger than Jupiter but only 91% of its mass completes a 3.4-day orbit at only 6.5 million km from its parent star
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Feb-19
Original link: https://pan.baidu.com/s/1WX4qhpUdv0tIEcAPe-Bdyg
"Open the pod-bay doors HAL"
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
- DaveBowman2001
- Posts: 772
- Joined: 06.07.2018
- Age: 24
- With us: 6 years 1 month
- Location: Manila, Philippines
WASP-13
The United Kingdom's Entry for NameExoWorlds (2019)
WASP-13, also known formally as Gloas, is a Sun-like star about 746.87 light-years away in the constellation Lynx. Its sole planet, Cruinlagh, is a gas giant larger than Jupiter but only half its mass, possibly indicating the absence of a planetary core at its interior. Both objects received their names from the second NameExoWorlds campaign in 2019
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Feb-19
Original link: https://pan.baidu.com/s/1WX4qhpUdv0tIEcAPe-Bdyg
The United Kingdom's Entry for NameExoWorlds (2019)
WASP-13, also known formally as Gloas, is a Sun-like star about 746.87 light-years away in the constellation Lynx. Its sole planet, Cruinlagh, is a gas giant larger than Jupiter but only half its mass, possibly indicating the absence of a planetary core at its interior. Both objects received their names from the second NameExoWorlds campaign in 2019
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Feb-19
Original link: https://pan.baidu.com/s/1WX4qhpUdv0tIEcAPe-Bdyg
"Open the pod-bay doors HAL"
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
- DaveBowman2001
- Posts: 772
- Joined: 06.07.2018
- Age: 24
- With us: 6 years 1 month
- Location: Manila, Philippines
Kepler-76
A Super-Jupiter with a 36-Hour Year
Kepler-76, also known as KOI-1658, is a F-type main sequence star about 2,749 light-years away in the constellation Cygnus. A large superjovian planet about 1.96 times the mass of Jupiter completes a 1.54-day orbit around its star at a distance of 4.1 million km
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: SolHorizon
Release date: 2023-Jan-12
Original link: https://pan.baidu.com/s/1onu65BNnjd9eZ9A0KNDYcQ
A Super-Jupiter with a 36-Hour Year
Kepler-76, also known as KOI-1658, is a F-type main sequence star about 2,749 light-years away in the constellation Cygnus. A large superjovian planet about 1.96 times the mass of Jupiter completes a 1.54-day orbit around its star at a distance of 4.1 million km
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: SolHorizon
Release date: 2023-Jan-12
Original link: https://pan.baidu.com/s/1onu65BNnjd9eZ9A0KNDYcQ
"Open the pod-bay doors HAL"
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
- DaveBowman2001
- Posts: 772
- Joined: 06.07.2018
- Age: 24
- With us: 6 years 1 month
- Location: Manila, Philippines
Kepler-1326
A Neptune with a Non-Existent Moon Half its Size
Kepler-1326, also known as KOI-2728, is an F-type subgiant star about 2,323 light-years away in the constellation Cygnus. A single neptunian planet is orbiting at a distance of 0.26 AU from its star once every 42 days, where in 2020 was speculated to harbor a massive satellite only half its size, but since deemed unlikely to exist according to follow-up studies
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Jan-9
Original link: https://pan.baidu.com/s/1O7iXzj3hwF-OOSDg51MUiA
A Neptune with a Non-Existent Moon Half its Size
Kepler-1326, also known as KOI-2728, is an F-type subgiant star about 2,323 light-years away in the constellation Cygnus. A single neptunian planet is orbiting at a distance of 0.26 AU from its star once every 42 days, where in 2020 was speculated to harbor a massive satellite only half its size, but since deemed unlikely to exist according to follow-up studies
This was retrieved from the Baidu site. Credits to the original author written down below.
Author: Pan-STARRS
Release date: 2023-Jan-9
Original link: https://pan.baidu.com/s/1O7iXzj3hwF-OOSDg51MUiA
"Open the pod-bay doors HAL"
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
"I'm sorry Dave, I'm afraid I can't do that"
Spacecrafts Addon Developer since 2018
Celestia Versions: 1.7.6 (Mobile), 1.6.4 and 1.7.0 (Windows)
- SevenSpheres
- Moderator
- Posts: 822
- Joined: 08.10.2019
- With us: 4 years 10 months
AU Microscopii
The nearest pre-main sequence planetary system
I've released an updated version of this system over in Nearby Exoplanets, as well as an update to Gliese 832.
The nearest pre-main sequence planetary system
I've released an updated version of this system over in Nearby Exoplanets, as well as an update to Gliese 832.
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
-
- Posts: 196
- Joined: 21.10.2021
- Age: 16
- With us: 2 years 10 months
- Location: Novo Hamburgo, State of Rio Grande do Sul, Brazil
UKIRT-2017-BLG-001L
UKIRT-2017-BLG-001L b is a gas giant exoplanet discovered in 2018 through gravitational microlensing. It is located 20,547 light years away from Earth, in the direction of the galactic center. It has 1.28 Jupiter masses and 1.22 Jupiter radius (estimate). It orbits its parent star every 9.5 Earth years at a distance of 4.18 AU.
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Texture created with the program "Textures for Planets"
Enjoy![Smile :smile:](./images/smilies/smile_real.gif)
UKIRT-2017-BLG-001L b is a gas giant exoplanet discovered in 2018 through gravitational microlensing. It is located 20,547 light years away from Earth, in the direction of the galactic center. It has 1.28 Jupiter masses and 1.22 Jupiter radius (estimate). It orbits its parent star every 9.5 Earth years at a distance of 4.18 AU.
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Texture created with the program "Textures for Planets"
Enjoy
![Smile :smile:](./images/smilies/smile_real.gif)
- Attachments
-
UKIRT-2017-BLG-001L.zip
- download
- (1.19 MiB) Downloaded 344 times
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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
LAWD 37
A WD planet in our backyard?
Download:
A WD planet in our backyard?
Download:
"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
- Trolligi 112477
- Posts: 259
- Joined: 18.04.2020
- Age: 16
- With us: 4 years 4 months
- Location: London
CWISE J0506+0738
CWISE J0506+0738
Another Beta Pic sub brown dwarf, a.k.a a "rogue planet"
R E D
Another Beta Pic sub brown dwarf, a.k.a a "rogue planet"
R E D
no more science papers
- Trolligi 112477
- Posts: 259
- Joined: 18.04.2020
- Age: 16
- With us: 4 years 4 months
- Location: London
TOI-2260
A potentially molten planet orbiting a young G-type star
TOI-2260 b and its host star
TOI-2260 is a young (0.321 Gyr), metal-rich (0.22 [Fe/H]) G-type star located about 330.23 lightyears away from the solar system, that star hosts an extremely hot super-Earth (1.62 Earth Radii) that completes an orbit every 8.4 hours. The star is one of the most metal-rich stars known that hosts an ultra-short period planet, additionally the planet itself is one of the hottest worlds that is less than 2 Earth Radii in size. The planet's mass has not been determined as of now.
A potentially molten planet orbiting a young G-type star
TOI-2260 b and its host star
TOI-2260 is a young (0.321 Gyr), metal-rich (0.22 [Fe/H]) G-type star located about 330.23 lightyears away from the solar system, that star hosts an extremely hot super-Earth (1.62 Earth Radii) that completes an orbit every 8.4 hours. The star is one of the most metal-rich stars known that hosts an ultra-short period planet, additionally the planet itself is one of the hottest worlds that is less than 2 Earth Radii in size. The planet's mass has not been determined as of now.
TOI-2096
Two eccentric planets with near-resonant orbits
the closely aligned worlds of TOI-2096
TOI-2096 is a red dwarf located about 158.04 lightyears away from the solar system. The star has two slightly eccentric planets orbiting it, a super-Earth (1.2 Earth Radii) and a sub-Neptune (1.9 Earth Radii). the planet's orbits are near a 2:1 MMR (mean-motion resonance), leading to the possibility of measuring the masses of these worlds via Transit Timing Variations. Additionally, the study that confirmed the planets believes it is possible for future atmospheric studies using JWST.
new version
Two eccentric planets with near-resonant orbits
the closely aligned worlds of TOI-2096
TOI-2096 is a red dwarf located about 158.04 lightyears away from the solar system. The star has two slightly eccentric planets orbiting it, a super-Earth (1.2 Earth Radii) and a sub-Neptune (1.9 Earth Radii). the planet's orbits are near a 2:1 MMR (mean-motion resonance), leading to the possibility of measuring the masses of these worlds via Transit Timing Variations. Additionally, the study that confirmed the planets believes it is possible for future atmospheric studies using JWST.
new version
Last edited by Karistus_ on 08.07.2023, 18:40, edited 2 times in total.
- Trolligi 112477
- Posts: 259
- Joined: 18.04.2020
- Age: 16
- With us: 4 years 4 months
- Location: London
- Trolligi 112477
- Posts: 259
- Joined: 18.04.2020
- Age: 16
- With us: 4 years 4 months
- Location: London
VHS 1256-1257
VHS 1256-1257
A very cloudy exoplanet orbiting two very low-mass objects
(The planet in the addon has moving clouds)
A very cloudy exoplanet orbiting two very low-mass objects
(The planet in the addon has moving clouds)
no more science papers
LTT 3780
Two planets of varying compositions around a red dwarf
LTT 3780 A's planets
LTT 3780, aka TOI-732, is a binary system composed of two red dwarfs located about 71.84 lightyears from the solar system. Two planets are currently known to orbit the primary component of the binary: a super-Earth on an ultra short period orbit and a mini-Neptune, LTT 3780 A b likely has a rocky dominated composition while LTT 3780 A c likely has a volatile rich envelope over a dense rocky core.
[Download] (14.3 mb)
Two planets of varying compositions around a red dwarf
LTT 3780 A's planets
LTT 3780, aka TOI-732, is a binary system composed of two red dwarfs located about 71.84 lightyears from the solar system. Two planets are currently known to orbit the primary component of the binary: a super-Earth on an ultra short period orbit and a mini-Neptune, LTT 3780 A b likely has a rocky dominated composition while LTT 3780 A c likely has a volatile rich envelope over a dense rocky core.
[Download] (14.3 mb)
Last edited by Karistus_ on 14.12.2023, 03:53, edited 1 time in total.
TOI-1246
4 Confirmed planets with varying densities and a fifth candidate
the four confirmed planets of TOI-1246
TOI-1246 is a binary system composed of a K-type star and a red dwarf located about 552.31 lightyears away from the solar system. The primary star has 4 confirmed planets orbiting at varying distances, 3 Neptunian planets (b= 3.01 Re, d= 3.51 Re, e= 3.78 Re), and an Oceanic planet (c= 2.51 Re). The masses of all these planets have been observed via Radial Velocity and TTVs of the outermost planets (b= 8.1 Me, c= 8.8 Me, d= 5.3 Me, e= 14.8 Me). The worlds vary in density with notable planets being TOI-1246 c with a composition >90% dominated by water and TOI-1246 d with a density nearly matching Saturn. Additionally, during the Radial Velocity observations of the system, an unlinked signal appeared. The study couldn't nail down if the signal is planetary or not, but if it is then it has a mass of 25.6 Me and orbits every 93.8 days
TOi-1246 f, the unconfirmed Neptune-like planet
confirmed planets
candidate planet
4 Confirmed planets with varying densities and a fifth candidate
the four confirmed planets of TOI-1246
TOI-1246 is a binary system composed of a K-type star and a red dwarf located about 552.31 lightyears away from the solar system. The primary star has 4 confirmed planets orbiting at varying distances, 3 Neptunian planets (b= 3.01 Re, d= 3.51 Re, e= 3.78 Re), and an Oceanic planet (c= 2.51 Re). The masses of all these planets have been observed via Radial Velocity and TTVs of the outermost planets (b= 8.1 Me, c= 8.8 Me, d= 5.3 Me, e= 14.8 Me). The worlds vary in density with notable planets being TOI-1246 c with a composition >90% dominated by water and TOI-1246 d with a density nearly matching Saturn. Additionally, during the Radial Velocity observations of the system, an unlinked signal appeared. The study couldn't nail down if the signal is planetary or not, but if it is then it has a mass of 25.6 Me and orbits every 93.8 days
TOi-1246 f, the unconfirmed Neptune-like planet
confirmed planets
candidate planet
Last edited by Karistus_ on 15.07.2023, 19:26, edited 1 time in total.
TOI-451
Three non-rocky worlds orbiting within a binary... or tertiary
All three worlds of TOI-451 A
TOI-451 is a young (120 Myr) binary (or tertiary?) star system consisting of a G-type star and 1 or 2 red dwarfs located about 403.39 light-years away from the solar system, the primary star hosts 3 Neptunian planets (b= 1.91 Re, c= 3.1 Re, d= 4.07 Re). The study also reported that they believe TOI-451 B is actually a binary of two equal-mass red dwarfs, but that's all they said about it.
Three non-rocky worlds orbiting within a binary... or tertiary
All three worlds of TOI-451 A
TOI-451 is a young (120 Myr) binary (or tertiary?) star system consisting of a G-type star and 1 or 2 red dwarfs located about 403.39 light-years away from the solar system, the primary star hosts 3 Neptunian planets (b= 1.91 Re, c= 3.1 Re, d= 4.07 Re). The study also reported that they believe TOI-451 B is actually a binary of two equal-mass red dwarfs, but that's all they said about it.
Last edited by Karistus_ on 10.07.2023, 06:49, edited 1 time in total.
TOI-1062
two hot eccentric worlds with a massive sub-Neptune
The hot worlds of TOI-1062
TOI-1062 is a G-type star located about 267.87 lightyears from the solar system. The star is accompanied by two planets, a rocky-dominate ocean planet (b= 2.27 Re) and a Neptunian planet (c= 9.78 Me). As mentioned earlier, TOI-1062 b's composition is likely dominated by a rocky core and mantle, with an outer liquid layer followed by an atmosphere, this gives the planet a mass of 10.15 Earth Masses. TOI-1062 c doesn't transit the star from our perspective so all we have is mass and we can't say for certain what its true composition is. Both worlds also have slightly eccentric orbits
[Download] (2.91 MB)
two hot eccentric worlds with a massive sub-Neptune
The hot worlds of TOI-1062
TOI-1062 is a G-type star located about 267.87 lightyears from the solar system. The star is accompanied by two planets, a rocky-dominate ocean planet (b= 2.27 Re) and a Neptunian planet (c= 9.78 Me). As mentioned earlier, TOI-1062 b's composition is likely dominated by a rocky core and mantle, with an outer liquid layer followed by an atmosphere, this gives the planet a mass of 10.15 Earth Masses. TOI-1062 c doesn't transit the star from our perspective so all we have is mass and we can't say for certain what its true composition is. Both worlds also have slightly eccentric orbits
[Download] (2.91 MB)
Last edited by Karistus_ on 30.08.2023, 21:31, edited 1 time in total.
TOI-712
Three mini Neptunes and a candidate rocky planet
Three mini-Neptunes of TOI-712
TOI-712 is a K-type star located about 191.10 light-years away from the solar system. The star has three planets, all mini-Neptunes orbiting at various distances (b= 2.049 Re, c= 2.701 Re, d= 2.474 Re). The orbits and distances of the planet vary with TOI-712 b having a close and eccentric orbit, though the eccentricity is poorly constrained, and the other two being farther out with TOI-712 d scrapping the edge of its star habitable zone. Additionally, during observations a fourth planet candidate was observed, it measured to be smaller than Earth and also has a close orbit (.05= 0.81 Re). The initial third candidate (TOI-712.03) was proven to be a false positive. There are no mass measurements for any of the planets.
There is a separate add-on for TOI-712.05
The rocky planet candidate of TOI-712
confirmed planets
condidate planet
Three mini Neptunes and a candidate rocky planet
Three mini-Neptunes of TOI-712
TOI-712 is a K-type star located about 191.10 light-years away from the solar system. The star has three planets, all mini-Neptunes orbiting at various distances (b= 2.049 Re, c= 2.701 Re, d= 2.474 Re). The orbits and distances of the planet vary with TOI-712 b having a close and eccentric orbit, though the eccentricity is poorly constrained, and the other two being farther out with TOI-712 d scrapping the edge of its star habitable zone. Additionally, during observations a fourth planet candidate was observed, it measured to be smaller than Earth and also has a close orbit (.05= 0.81 Re). The initial third candidate (TOI-712.03) was proven to be a false positive. There are no mass measurements for any of the planets.
There is a separate add-on for TOI-712.05
The rocky planet candidate of TOI-712
confirmed planets
condidate planet
Last edited by Karistus_ on 11.07.2023, 04:20, edited 2 times in total.