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Home , 55 Cancri e, Carbon planet, Gliese 1132 b, Gliese 1214, Gliese 22, Gliese 69

scaled one in 120 million 3D MODEL ONLY

tato_713

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updated 5. 3. 2021 | published 5. 3. 2021

Summary

Some of the notable -sized exoplanets scaled (smaller than 2.5 Earth diameter).

Learning > Physics & Astronomy

trappist1h trappist1g trappist1f trappist1e trappist1d trappist1c trappist1b trappist1 trappist terrestrialplanet space scalemodel scaledmodel scale proximacentauri planetas planeta oceanworld kepler62b kepler62 kepler22b kepler22 kepler11b icegigant extraterrestrial corot7 chthonianplanet chthonian astronomy astronomia

Originally published here: Exoplanets scaled one in 120 million by tato_713 - Thingiverse

The concept of this post is to compare the size in the same scale of various Earth sized exoplanets with the Earth itself or other astronomical bodies like . Although there are thousands exoplanets confrmed, I made only some of the most notorious ones with known diameter, and nearly Earth sized (up to 2.5 its diameter). The models are just spheres scaled one in 120 million, to compare with terrestrial planets; one in 250 million; and one in 500 million for the biggest ones.

The fle's names explained: name_1_x_10_y.stl is 1 : x* 10^y. So _1_6_10_7 is 1:600000000 or one in 60 million.

Proxima Centauri b

Proxima b is the closest known to the , the closest within the habitable zone of its , the only known planet in the nearest star, , and the only one confrmed in the system. As is it said, the host star for the planet is part of the Alpha Centauri system, orbiting the two main Alpha Centauri A (Rigil Kentaurus) and B (Toliman). Proxima is a fare M type while the others are G ( like) and K type (orange star) respectively. Flare stars are randomly emit huge fares that could have devastating efects on a close planet , unless it has a strong magnetic feld.

• Type: Planet. • Orbit: Proxima Centauri. • Distance to the Sun: 4.244 ly. • : 11.186 d • Composition: Silicate rock. • : ~5 g/cm3. • Dimensions: ~14000 km • Model scale: 1:1.2x108 (11cm) 1:2.5x108 (5cm)

Luyten b

Luyten b is the fourth closest planet in the habitable zone. It's orbiting the Luyten's Star, which is a red dwarf, that unlike Proxima Centauri, it's relatively inactive. This planet is classifed as a super-Earth, a planet bigger than Earth, but smaller than Neptune, it isn't related with its composition.

• Type: Planet. • Orbit: Luyten's Star. • Distance to the Sun: 12.2 ly. • Orbital period: 18.6498 d • Composition: Silicate rock. • Density: ~6 g/cm3. • Dimensions: ~17000 km • Model scale: 1:1.2x108 (14cm) 1:2.5x108 (7cm) HD 219134 b

This planet was at the time of its discovery, the closest known rocky planet. It a K type star. It is in the hot zone of its system, which means that cannot be liquid on its surface. It is one of the few exoplanets with a detected atmosphere. The star is visible to the naked eye, and is one of the oldest star know with 11 billion of .

• Type: Planet. • Orbit: HD 219134 • Distance to the Sun: 21.25 ly. • Orbital period: 3.092926 d • Composition: Silicate rock. • Density: ~6.4 g/cm3. • Dimensions: ~20400 km • Model scale: 1:1.2x108 (17cm) 1:2.5x108 (8cm)

HD 219134 c

The HD 219134 system has at least 5, and possibly 7, planets; of which the two most close to the star has known diameter. HD 219134 c is the second one, also with a possible atmosphere. The rest of the planets of this system are also more massive.

• Type: Planet. • Orbit: HD 219134 • Distance to the Sun: 21.25 ly. • Orbital period: 6.76458 d • Composition: Silicate rock. • Density: ~7 g/cm3. • Dimensions: ~19250 km • Model scale: 1:1.2x108 (16cm) 1:2.5x108 (8cm)

Gliese 1132 b

• Type: Planet. • Orbit: Gliese 1132. • Distance to the Sun: 39 ly. • Orbital period: 1.6 d • Composition: Silicate rock. • Density: ~6.3 g/cm3. • Dimensions: ~14500 km • Model scale: 1:1.2x108 (12cm) 1:2.5x108 (6cm) Trappist-1 b

Trappist-1 is one of the best studied exoplanets. It has 7 Earth sized planets that in front of the host star, viewed from the Solar System. It is an ultra-cool red dwarf slightly larger than . All of the planets orbits very close to the star, comparable with the distance between the Earth and the Moon, so a planet of the system is visible from the surface of the others. The planet b (the closest to the star) has a like atmosphere mainly composed of CO2 and it is inferred to have because of its low density.

• Type: Planet. • Orbit: Trappist-1. • Distance to the Sun: 39.6 ly. • Orbital period: 1.51 d • Composition: Silicate rock. Water vapor and CO2 atmosphere • Density: ~4 g/cm3. • Dimensions: ~14200 km • Model scale: 1:1.2x108 (12cm) 1:2.5x108 (6cm)

Trappist-1 c

Trappist-1 c is, like the b, a Venus like planet with water vapor atmosphere, too hot to be liquid. Like most if not all the planet on the system it is likely tidal locked to the star.

• Type: Planet. • Orbit: Trappist-1. • Distance to the Sun: 39.6 ly. • Orbital period: 2.42 d • Composition: Silicate rock. • Density: ~4.8 g/cm3. • Dimensions: ~14000 km • Model scale: 1:1.2x108 (11cm) 1:2.5x108 (5cm)

Trappist-1 d

Trappist-1 d is the smallest and less densest planet of the Trappist-1 system. It is between the size of and Earth. This planet orbits the inner edge of the habitable zone, but it is likely tidal locked.

• Type: Planet. • Orbit: Trappist-1. • Distance to the Sun: 39.6 ly. • Orbital period: 4.049 d • Composition: Silicate rock. • Density: ~3.4 g/cm3. • Dimensions: ~10000 km • Model scale: 1:1.2x108 (8cm) 1:2.5x108 (4cm)

Trappist-1 e

The e planet is one of the most Earth like one know, well within the habitable zone, slightly smaller, and nearly the same density of our planet. The habitability of the red dwarf planets is cuestionable, mostly because of the tidal lock. The always- hemisphere may be too hot, while the night one may be too cold. It could be that in the border line between the hemispheres, the air is warm enough to sustain Earth like conditions. Also if the atmosphere is thick enough, it could distribute more efciently the air .

• Type: Planet. • Orbit: Trappist-1. • Distance to the Sun: 39.6 ly. • Orbital period: 6.099 d • Composition: Silicate rock. • Density: ~5.6 g/cm3. • Dimensions: ~11500km • Model scale: 1:1.2x108 (9cm) 1:2.5x108 (4cm)

Trappist-1 f

Trappist-1 f is about the size of Earth, but two third its . This low density is consistent with a water rich world (20% of its mass, contrast to the 0.02% of Earth's mass). This means that it is probably an world, with a combination of water vapor atmosphere, liquid ocean and large ice blocks.

• Type: Planet. • Orbit: Trappist-1. • Distance to the Sun: 39.6 ly. • Orbital period: 9.2 d • Composition: Silicate rock. ?. • Density: ~4.5 g/cm3. • Dimensions: ~13300 km • Model scale: 1:1.2x108 (11cm) 1:2.5x108 (5cm)

Trappist-1 g

Like other members of this system, Trappist-1 g appear to be composed of high amounts of water, in this case in form of ices. It is the biggest planet of the system, although most of them are similar in size. Because of their proximity, the planet of the Trappist-1 system are locked in an , similar to the , , and .

• Type: Planet. • Orbit: Trappist-1. • Distance to the Sun: 39.6 ly. • Orbital period: 12.354 d • Composition: Silicate rock, and ice. • Density: ~4 g/cm3. • Dimensions: ~14500 km • Model scale: 1:1.2x108 (12cm) 1:2.5x108 (6cm)

Trappist-1 h

The h planet is the outermost one of the Trappist-1 system. It has about the same size and density of that of Mars, but is though to be composed 5% of water ice. It is unlikely that this has many bigger planets in larger orbits, because their efects on the star light must be detectable, as well as their transits in front of the star.

• Type: Planet. • Orbit: Trappist-1. • Distance to the Sun: 39.6 ly. • Orbital period: 18.767 d • Composition: Silicate rock, and ice. • Density: ~4 g/cm3. • Dimensions: ~10000 km • Model scale: 1:1.2x108 (8cm) 1:2.5x108 (4cm)

( e) Janssen

55 Cancri was one of the frsts to be discovered with more than two exoplanets. It is system of a K type star (55 Cancri A), which has all the 5 known planets of the system, and a smaller M type red dwarf (55 Cancri B). Only the e planet of this system, nicknamed Janssen, has a known radius, because its proximity to the star makes possible the transits. It could be a planet, a planet composed of silicate rock and core like Earth, but with a thick crust and of carbonaceous material. This hypothetical type of planet may have layers of and below its surface, and high amount of like in the surface, as well as , dioxide, and smog in the atmosphere. In the Solar system there aren't large carbon based bodies, only the C-type (like 253 Mathilde) are mainly composed of carbonaceous material.

• Type: Planet. • Orbit: Copernicus. • Distance to the Sun: 41.06 ly. • Orbital period: 17 hr 40 min • Composition: . • Density: ~6.7 g/cm3. • Dimensions: ~23900 km • Model scale: 1:1.2x108 (20cm) 1:2.5x108 (9cm)

Gliese 1214 b

Because its low density Gliese 1214 b could be mainly water in composition. Ocean worlds are theorised to have a thick ice layer at the bottom the ocean, that prevents the exchange of other-than-water nutrients from the mantle, which left poor conditions for the life as we know. Gliese 1214 b could also be a smaller version of ice giants like Neptune and .

• Type: Planet. • Orbit: Gliese 1214. • Distance to the Sun: 47.8 ly. • Orbital period: 1.58 d • Composition: Ocean world. • Density: ~1.88 g/cm3. • Dimensions: ~34000 km • Model scale: 1:2.5x108 (14cm) 1:5x108 (7cm)

Kepler-37 b

Kepler-37 b at the time of its discovery was the smallest planet know. It is also the smallest one known to orbit a Sun like star. It is a bit larger than the Moon. By its proximity to the star and the small size it is likely to be rocky in composition, like the moon, but the exact composition is unknown yet because the mass and density of any planet of the system cannot be determined.

• Type: Planet. • Orbit: Kepler-37. • Distance to the Sun: 209 ly. • Orbital period: 13.367 d • Composition: Terrestrial. • Density: ~1.24 g/cm3. • Dimensions: ~3900 km • Model scale: 1:1.2x108 (4cm) 1:2.5x108 (2cm) Kepler-37 c

• Type: Planet. • Orbit: Kepler-37. • Distance to the Sun: 209 ly. • Orbital period: 21.302 d • Composition: Terrestrial. • Density: ? g/cm3. • Dimensions: ~9450 km • Model scale: 1:1.2x108 (8cm) 1:2.5x108 (4cm)

Kepler-37 d

• Type: Planet. • Orbit: Kepler-37. • Distance to the Sun: 209 ly. • Orbital period: 39.792 d • Composition: Terrestrial. • Density: ? g/cm3. • Dimensions: ~25000 km • Model scale: 1:1.2x108 (21cm) 1:2.5x108 (10cm)

COROT-7 b

COROT-7 b was the frst planet known to be terrestrial. Because its proximity to the COROT-7 star and its high density, it is a candidate for a chthonian planet, an hypothetical kind of planet that is the remnant rocky core of an ice or which atmosphere was stripped of by the stellar winds.

• Type: Planet. • Orbit: COROT-7. • Distance to the Sun: 489 ly. • Orbital period: 20 h 29 min. • Composition: Chthonian planet. • Density: ~7.5 g/cm3. • Dimensions: ~20100 km • Model scale: 1:1.2x108 (17cm) 1:2.5x108 (8cm)

BD +20 594 b

BD+20594 b is the 594th entry in the +20° zone of the Bonner catalogue (the "b" is because is the frst planet of the system); in the Kepler program is K2-56, indicating that it is from the second part of the program. It is one of the proposed mega-Earth. Contrary to the term "super-Earth" that reference only the size, mega are planets 2 or more times the Earth radius, that are composed of terrestrial compounds, that is, they are not gas gigant, and have a perceptible interface between the gas and liquid.

• Type: Planet. • Orbit: BD +20 594. • Distance to the Sun: 496.08 ly. • Orbital period: 41.68 d • Composition: Silicate rock. • Density: 7.89 g/cm3. • Dimensions: ~28400 km • Model scale: 1:2.5x108 (11cm) 1:5x108 (6cm)

WD 1145+017 b

This is the frst planet known around a . It is also the smaller planetary object, being smaller than , so it is not guaranteed that it meets the requirements for being a planet. It can be vaporizing by in host remnant star. Life conditions around a white dwarf are unclear, the of these bodies is too weak, so the habitable zone is too short. Also, volatile materials like water and may have being eroded by . White dwarf are usually the size of Earth, so transits in front of them are rare. The host white dwarf of this planetary object is posted here.

• Type: ? • Orbit: WD 1145+017. • Distance to the Sun: 570 ly. • Orbital period: 4 h 30 min • Composition: Terrestrial? • Density: ~1 g/cm3. • Dimensions: ~1900 km • Model scale: 1:1.2x108 (1.4cm)

Kepler-10 b

Kepler-10 b was the frst planet confrmed to be a . Like most of the planets discovered by transit method, it orbits very close to its host star. This is because this method is extremely biased to this kind of planets. It is very likely that Kepler-10 b has a dry surface, like that of .

• Type: Planet. • Orbit: Kepler-10. • Distance to the Sun: 608 ly. • Orbital period: 20 h 6 min • Composition: Terrestrial. • Density: ~5.8 g/cm3. • Dimensions: ~18700 km • Model scale: 1:1.2x108 (15cm) 1:2.5x108 (7cm)

Kepler-10 c

Kepler-10 c is probably a mini-Neptune, a super-Earth with the composition of that of ice giants. It also sometimes applies to hydrogen planets smaller than Neptune. For these planets, the term "gas dwarf" may be more accurate.

• Type: Planet. • Orbit: Kepler-10. • Distance to the Sun: 608 ly. • Orbital period: 45.295 d • Composition: Terrestrial or . • Density: ~3.1 g/cm3. • Dimensions: ~30000 km • Model scale: 1:2.5x108 (12cm) 1:5x108 (6cm)

Kepler-22 b

Although the exact mass of this planet is unknown, it's thought to be an ocean planet, a theoretical kind of planet dominated by water ocean environment.

• Type: Planet. • Orbit: Kepler-22. • Distance to the Sun: 638 ly. • Orbital period: 289.862 d • Composition: Ocean world. • Density: ? g/cm3. • Dimensions: ~30600 km • Model scale: 1:2.5x108 (12cm) 1:5x108 (6cm)

EPIC 201497682 b

One of the smallest and recent planets discovered. It is too close to its star, so it's uninhabitable.

• Type: Planet. • Orbit: EPIC 201497682. • Distance to the Sun: 831 ly. • Orbital period: 2.1 d • Composition: Terrestrial. • Density: ~4.3 g/cm3. • Dimensions: ~8800 km • Model scale: 1:1.2x108 (7cm) 1:2.5x108 (3.5cm)

Kepler-62 b

Kepler 62 is a 5 known planet system K-type star. This kind of star is an intermediate between M-type red dwarf and G-type Sun-like star, called "dwarf orange". The lighter the star, the longer its life. Their life is longer to that of Sun like stars, and they are less likely to have the problems of red dwarfs, like the of the planet and the probability of being a fare star. The b planet is a typical super-Earth planet, in the hot zone of the star.

• Type: Planet. • Orbit: Kepler-62. • Distance to the Sun: 990 ly. • Orbital period: 5.715 d • Composition: Terrestrial. • Density: ~5.15 g/cm3. • Dimensions: ~16700 km • Model scale: 1:1.2x108 (14cm) 1:2.5x108 (7cm)

Kepler-62 c c is a Mars sized exoplanet with the stellar fux of that of Mercury.

• Type: Planet. • Orbit: Kepler-62. • Distance to the Sun: 990 ly. • Orbital period: 12.44 d • Composition: Terrestrial. • Density: ~3.5 g/cm3. • Dimensions: ~6900 km • Model scale: 1:1.2x108 (6cm) 1:2.5x108 (3cm)

Kepler-62 d d is the biggest planet known of the system, and orbits in the "Venus zone" of the star, where the planet is too hot for having liquid water in its surface, but it is not close enough to deplete its atmosphere. By its density it is something between a small version of Neptune and a gigant version of Venus.

• Type: Planet. • Orbit: Kepler-62. • Distance to the Sun: 990 ly. • Orbital period: 18.164 d • Composition: Terrestrial or ice giant. • Density: ~4 g/cm3. • Dimensions: ~24800 km • Model scale: 1:1.2x108 (20cm) 1:2.5x108 (10cm)

Kepler-62 e e is in the limit of size (1.6 Earth's ) in which a planet is expected to be a big rocky planet or an small gaseous planet. It lays within the habitable zone.

• Type: Planet. • Orbit: Kepler-62. • Distance to the Sun: 990 ly. • Orbital period: 122.387 d • Composition: Terrestrial or ice giant. • Density: ~5.9 g/cm3. • Dimensions: ~20500 km • Model scale: 1:1.2x108 (17cm) 1:2.5x108 (8cm)

Kepler-62 f f orbits in the outer part of the habitable zone of its star, meaning that it could be covered of ice if it hasn't a substancial atmosphere to retain the heat.

• Type: Planet. • Orbit: Kepler-62. • Distance to the Sun: 990 ly. • Orbital period: 267.29 d • Composition: Terrestrial. • Density: ~5.5 g/cm3. • Dimensions: ~18000 km • Model scale: 1:1.2x108 (15cm) 1:2.5x108 (7cm)

Kepler-452 b "Coruscant"

Sometimes called "Earth 2.0", this planet is important because is the frst nearly certain terrestrial planet orbiting whit in the habitable zone of a G- type star. The orbital period is similar to that of Earth. This kind of planet are difcult to detect since planets that far from its star are less likely to transit in front of the star viewed from Earth.

• Type: Planet. • Orbit: Kepler-452. • Distance to the Sun: 1402 ly. • Orbital period: 384.843 d • Composition: Terrestrial. • Density: ~4.18 g/cm3. • Dimensions: ~14100 km • Model scale: 1:1.2x108 (11cm) 1:2.5x108 (5cm)

Kepler-145 b

Another candidate for being a mega-Earth planet.

• Type: Planet. • Orbit: Kepler-145. • Distance to the Sun: 1848.5 ly. • Orbital period: 11.186 d • Composition: Terrestrial. • Density: ~11 g/cm3. • Dimensions: ~33800 km • Model scale: 1:2.5x108 (13cm) 1:5x108 (6cm)

Kepler-11 b

The Kepler-11 system is compact compared with Solar System, althogh there could be more planets that not transit the star. All the 6 known planets orbit within the orbit of Venus. The star is G-type, slithly heavier that the Sun. All the planets are bigger than the Earth, and the biggest, about the size of Neptune or Uranus.

• Type: Planet. • Orbit: Kepler-11. • Distance to the Sun: 2150 ly. • Orbital period: 10.304 d • Composition: Water. • Density: ~1.8 g/cm3. • Dimensions: ~22900 km • Model scale: 1:1.2x108 (19cm) 1:2.5x108 (9cm) 1:5x108 (4cm)

Kepler-11 c

• Type: Planet. • Orbit: Kepler-11. • Distance to the Sun: 2150 ly. • Orbital period: 13.024 d • Composition: Water. • Density: ~1.7 g/cm3. • Dimensions: ~36500 km • Model scale: 1:2.5x108 (14cm) 1:2.5x108 (7cm)

Kepler-11 f

Type: Planet. Gas dwarf.

• Orbit: Kepler-11. • Distance to the Sun: 2150 ly. * • Orbital period: 46.689 d * • Composition: Volatile materials.. * • Density: ~0.7 g/cm3. * • Dimensions: ~31700 km * • Model scale: 1:2.5x108 (13cm) 1:2.5x108 (6cm)

Kepler-69 b

• Type: Planet. • Orbit: Kepler-69. • Distance to the Sun: 2430 ly. • Orbital period: 13.722 d • Composition: Terrestrial or ice giant. • Density: ? g/cm3. • Dimensions: ~28500 km • Model scale: 1:2.5x108 (11cm) 1:5x108 (6cm)

Kepler-69 c

This is a super-Earth planet in a Venus-like orbit around a Sun-like star.

• Type: Planet. • Orbit: Kepler-69. • Distance to the Sun: 2430 ly. • Orbital period: 242.461 d • Composition: Terrestrial. • Density: ? g/cm3. • Dimensions: ~21800 km • Model scale: 1:1.2x108 (18cm) 1:2.5x108 (9cm) 1:5x108 (4cm)

Kepler-90 b

This system is known for being analogous in planet distribution to the Solar System. It has 8 known planets, the frst 3 are likely terrestrial, the next 3 are in the range of super-Earth size, and the last 2 are jovian planets by they size. It is one of the farthest known multiple planet system discovered by the Kepler mission.

• Type: Planet. • Orbit: Kepler-90. • Distance to the Sun: 2840 ly. • Orbital period: 7 d • Composition: Terrestrial. • Density: ? g/cm3. • Dimensions: ~16700 km • Model scale: 1:1.2x108 (14cm) 1:2.5x108 (7cm)

Kepler-90 c

• Type: Planet. • Orbit: Kepler-90. • Distance to the Sun: 2840 ly. • Orbital period: 8.719 d • Composition: Terrestrial. • Density: ? g/cm3. • Dimensions: ~15000 km • Model scale: 1:1.2x108 (13cm) 1:2.5x108 (6cm)

Kepler-90 i

This planet is known for being discovered using a machine learning algorithms on the transit data.

• Type: Planet. • Orbit: Kepler-90. • Distance to the Sun: 2840 ly. • Orbital period: 14.449 d • Composition: Terrestrial. • Density: ? g/cm3. *Dimensions: ~16800 km • Model scale: 1:1.2x108 (14cm) 1:2.5x108 (7cm)

OGLE-2005-BLG-390L b "Hoth"

This planet is one of the frst, and the few, Earth-like planet discovered using gravity microlesing, the detection of the lens efect that a exoplanet does of a background star. This method allows to detect planets with long orbital period, because they must be separated enough of they stars. Prior to the Kepler mission it was the most Earth-like exoplanet known.

• Type: Planet. • Orbit: OGLE-2005-BLG-390L. • Distance to the Sun: 21500 ly. • Orbital period: ~10 yr • Composition: Terrestrial or ice giant. • Density: ~6.3 g/cm3. • Dimensions: ~21500 km • Model scale: 1:1.2x108 (18cm) 1:2.5x108 (9cm)

Other astronomical objects

Inner Solar System

Artifcial

Near Earth Asteroids

Main Belt Asteroids

Jovian System

Saturn System

Uranian System

Neptunian System

Centaurs

Comets

Trans Neptunian Objects

Extrasolar Objects

Sky Maps

Ancient

Speculative

Science Fiction

F3 Model Files (.stl, .3mf, .obj, .amf) 3D DOWNLOAD ALL FILES

55cancri_e_half_1_12_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021 trappist1_h_1_25_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler90_i_half_1_12_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

kepler69_b_half_1_25_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

kepler22_b_half_1_5_10_8.stl 222.1 KB F3 3D updated 4. 3. 2021

kepler22_b_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

proxima_b_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

hd219134_c_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler11_c_half_1_25_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

kepler11_f_1_5_10_8.stl 406.3 KB F3 3D updated 4. 3. 2021 kepler10_b_1_25_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler37_d_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler90_b_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

trappist1_g_1_25_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler69_c_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler62_b_half_1_25_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

kepler11_b_1_5_10_8.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler90_i_half_1_25_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

trappist1_f_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021 trappist1_g_half_1_25_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

trappist1_f_half_1_25_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

kepler90_b_half_1_12_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

kepler145_b_half_1_25_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

kepler90_i_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler11_b_1_25_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler145_b_half_1_5_10_8.stl 222.1 KB F3 3D updated 4. 3. 2021

proxima_b_half_1_25_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

trappist1_f_half_1_12_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021 ogle2005blg390l_b_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

trappist1_e_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler62_b_half_1_12_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

kepler37_c_1_25_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler90_i_1_25_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler452_b_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler62_e_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

proxima_b_1_25_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

gliese1214_b_1_5_10_8.stl 406.3 KB F3 3D updated 4. 3. 2021 kepler22_b_1_5_10_8.stl 406.3 KB F3 3D updated 4. 3. 2021

kepler62_e_1_25_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

bd20594_b_1_5_10_8.stl 406.3 KB F3 3D updated 4. 3. 2021

epic20147682_b_half_1_25_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021

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kepler62_f_half_1_12_10_7.stl 222.1 KB F3 3D updated 4. 3. 2021 trappist1_c_1_12_10_7.stl 406.3 KB F3 3D updated 4. 3. 2021

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