HD 189733 A b heat map scaled one in one billion

This is the first exoplanet with its global surface mapped in any way. The map is an infrared emission map, that is the radiation from its surface temperature. It has nothing to do with global shape or topography; it is a tidal locked gas planet, so its true shape is spherical, more spherical than Solar System gas giant Jupiter or Saturn, since its longer rotational period. It could be assumed that while hotter the place, more inflated the atmosphere is, so higher is the relief. If this is true, the topography in this model is still extremely exaggerated to make it more noticeable, about 15% of the radius, giving the model an egg shape. The star-facing direction (since it is tidal locked) of every model in this post is the positive X-axis. For Earth sized exoplanets, see this.
The file'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.

HD 189733 A b

This is the closest know transiting hot Jupiter, about 1.14 times Jupiter's diameter, and it's one of the best studied of this kind of planet. A hot Jupiter is a planet of jovian size (bigger than Saturn) that orbits very close to its star. It's tidal locked, as expected in planets orbiting that close. It orbit the main star of a binary system, a orange K-type star and a red M-type dwarf. The infrared emission indicates that the hottest longitude is 30° west to the star-facing meridian. This is because the day to night gas redistribution; with winds up to supersonic speeds. By the spectre of the planet, is know to be blue, and it's probably sign of presence of silicate material within its atmosphere. This led to the speculation that it may have "rains of molten glass" within it. This planet has the most depth transit of its star viewed from Earth, and it was possible to detect the volatile escaping from it.

• Type: Planet.
• Orbit: HD 189733 A.
• Distance to the Sun: 64.5 ly.
• Orbital period: 2 d 5 h 15 min
• Composition: Water vapor, oxygen, organics and silicate materials.
• Density: ~0.98 g/cm³.
• Dimensions: ~162000 km
• Model scale: 1:1x10⁹ (16cm)

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
Hygiea	2M, 4M, 10M
Antiope	1M, 2M
Jovian System
Jupiter	500M, 1G
Amalthea	2M, 4M
Thebe	1M, 2M
Io	20M, 60M
Europa	20M, 60M
Ganymede	60M, 120M
Callisto	60M, 120M
Saturn System
Saturn	500M, 1G
Pan, Daphnis and Atlas	80K, 200K, 500K, 1M
Prometheus and Pandora	1M, 2M
Janus and Epimetheus	2M, 4M
Mimas	2M, 4M, 10M
Methone, Anthe and Pallene	40K, 80K
Enceladus	4M, 10M
Tethys	4M, 10M, 20M
Telesto and Calypso	200K, 500K
Dione	4M, 10M, 20M
Helene	500K, 1M
Rhea	10M, 20M
Titan	60M, 120M
Hyperion	2M, 4M
Iapetus	10M, 20M
Phoebe	1M, 2M, 4M
Uranian System
Uranus	250M, 500M, 1G
Puck	1M, 2M, 4M
Miranda	4M, 10M
Ariel	10M, 20M
Umbriel	10M, 20M
Titania	10M, 20M
Oberon	10M, 20M
Neptunian System
Neptune	250M, 500M, 1G
Larissa	2M, 4M
Proteus	2M, 4M, 10M
Triton	20M
Comets
Tempel 1	40K, 80K, 200K
Wild 2	40K, 80K
Churyumov-Gerasimenko	20K, 40K, 80K
Hartley 2	20K, 40K, 80K
Borrelly	40K, 80K, 200K
Halley	80K, 200K
Centaurs and TNOs
Hidalgo	500K, 1M
Chariklo	2M, 4M
Pluto and Charon	10M, 20M
Styx, Nix, Kerberos and Hydra	500K, 1M
Haumea, Namaka and Hiʻiaka	10M, 20M
Arrokoth	200K, 500K, 1M
Largest TNOs and their moons	10M, 20M
Extrasolar
Exoplanets	120M, 250M, 500M
Nearest white dwarfs	120M, 250M
HD 189733 b	1G
Pulsars	200K, 500K
Cygnus X-1 accretion disk	10M, 20M
Sky maps
Heliosphere	7.5*1013, 1.5*1014
Constellations	-
CMBR	2*1028
Ancient
Earth (540 Mya to 20 Mya)	60M, 120M, 250M
Luna (4 Gya)	20M, 60M
Speculative
Planet Nine	250M, 500M
Cube planet	60M, 120M, 250M
Science Fiction
Ghroth	4M, 10M
Arda	60M, 120M
B612	10, 20, 32, 40
Mesklin	500M, 1G
Arrakis	60M, 120M
Borg cube	8K, 20K, 40K
Pern	60M, 120M
Europa Monolith	200K, 500K
Leonora Christine	500, 600, 1K, 3K
Rama	80K, 200K, 500K
Death Star	500K, 1M, 2M
Starkiller Base	2M, 4M, 10M
Nirn, Secunda and Masser	20M, 60M, 120M
Independence Day mothership	2M, 4M, 10M
Arrival heptapod spaceship	1K, 3K, 8K
Gaijin flowership	3K
Halo Array	4M, 10M, 20M, 60M
Gem Homeworld	120M, 250M, 500M
The Skeld	40, 80, 160, 350, 500
Misc
Mars (1962 reconstruction)	60M, 120M
Flat Earth	250M
Expanding Earth	60M, 120M
Spaceship of Ezekiel	80, 160