These models were rendered using MATLAB R2016a the data of the Rosetta spacecraft from the PDS site. The file's names explained: name_1_x_10_y.stl is 1 : x * 10y. So _1_6_10_7 is 1:600000000 or one in 60 million.
2867 Šteins
This small asteroid is part of the backround population, asteroids that do not form part of any family. It is an E-type asteroid, a relatively rare type from the inner belt. These asteroids may be part of a primordial belt, the E belt, that were scattered during the Late Heavy Bombardment.
Type: Asteroid.
Orbit: Sun. Main Asteroid Belt.
Orbital period: 3.63 yr.
Composition: Enstatite rock. E type
Density: ? g/cm3.
Dimensions: 6.83 km × 5.70 km × 4.42 km
Model scale: 1:4x104 (17cm) 1:8x104 (9cm) 1:2x105 (3.4cm)
References
"Farnham, T.L., Jorda, L., SHAPE MODEL OF ASTEROID 2867 STEINS, RO-A-OSINAC/OSIWAC-5-STEINS-SHAPE-V1.0, NASA Planetary Data System, 2013."
Surf to STL function for MATLAB
Other astronomical objects
Object
Scale [1:x]
K = 103 (thousand)M = 106 (million)G = 109 (billion)
Image
Inner Solar System
Mercury
20M, 60M,
120M
Venus
60M,
120M,
250M
Earth
60M,
120M,
250M
Luna
10M, 20M,
60M
Mars
20M, 60M,
120M
Phobos and Deimos
200K,
500K
Artificial
Salyut 7
40, 48, 80, 160
Near Earth Asteroids
Moshup and Squannit
8K,
20K,
40K
Ra-Shalom
20K,
40K
Castalia
8K,
20K,
40K
Bacchus
8K,
20K
Bennu
3K,
8K
Ryugu
3K, 8K,
20K
Geographos
40K,
80K
Phaethon
40K,
80K
Itokawa
3K,
8K
Eros
80K, 200K,
500K
Nereus
3K,
8K
Mithra
20K,
40K
Golevka
8K
Toutatis
40K,
80K
Main Asteroid Belt
Gaspra
200K
Annefrank
40K,
80K
Braille
20K,
40K
Vesta
2M, 4M,
10M
Šteins
40K,
80K,
200K
Iris
2M,
4M
Hebe
1M,
2M,
4M
Lutetia
500K, 1M,
2M
Julia
1M,
2M,
4M
Mathilde
500K,
1M
Juno
2M,
4M
Ceres
4M,
10M
Pallas
4M,
10M
Kleopatra
2M,
4M
Ida
500K,
1M
Psyche
2M,
4M
Interamnia
2M,
4M
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