243 Ida scaled one in one million

cults3d

This model was rendered using MATLAB R2016a on the ICQ model of the PSI made by Peter Thomas from the data of the Galileo mission. 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. 243 Ida Ida was the second asteroid visited by a spacecraft, the flyby was made by the Galileo probe in its way to Jupiter. It was the second minor planet to be discovered to have a satellite, named Dactyl. It is a S type asteroid, which means that is composed of silicate rock. It is one of the biggest member of the Koronis family. Asteroids families are group of them that share orbital and spectral characteristics, and are the result of a collision that shattered apart the main body into various pieces. Type: Asteroid. Koronis family. Orbit: Sun. Main Asteroid Belt. Orbital period: 4.8395 yr. Composition: Silicate rock. S type Density: 2.6 g/cm3. Dimensions: 59.8 km × 25.4 km × 18.6 km Model scale: 1:5x105 (12cm) 1:1x106 (6cm) References "https://sbn.psi.edu/pds/resource/oshape.html" 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, <a href="/tato_713/collections/one-in-four-