1P/Halley scaled one in 200 thousand

This model was rendered using MATLAB R2016a on the ICQ model of the PSI made by Philip Stooke. With this model I've try a modification of the surf2stl function I use for all the models, along with the interpolation method I have described here. Like many, if not all, comets its rotation is chaotical and may change over the time, so the northern and southern hemispheres cannot be determined, and the labels "north" and "south" in the model's file names and the model inclination are arbitrary.
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.

1P/Halley

Halley's comet is the only naked-eye visible short periodic comet, most of the comets seen have periods of thousand of years, and most of the periodic comets are too small and faint to be seen. This comet was the first one to be identificated as periodic, by Edmond Halley, and can be tracked back to 240 BC in ancient records. Short period comets are though to be former Kuiper belt and Scattered disk objects that fall down into a highly elliptical, Jupiter resonant, orbit. They could be, but it is unusual, deorbited long period comets, which origin is in the hypothetical Oort cloud. Halley's comet has one of the biggest known nucleus of any comet. The nucleus of a comet (the solid part) is composed of water ice, dust particles and organic compounds. Arrokoth may be a prototype of a cometary body before the perturbation from another object makes it fall into a lower orbit. When any comet come close to the inner Solar System, the volatile material sublimates and creates an atmosphere, that elongates in the oposite direction of the Sun, because of the solar wind, creating the coma of the comet. The dust impulsed by the thrown material creates the tail. Comets come so close to the Sun that they could be destroyed, evaporating completely, or breaking apart into smaller pieces, that could coalesce again to a weak rubble pile or create a new comet family. A comet could eventually impact with a planets or other objects, like the comet Shoemaker - Levy 9 which collided with Jupiter after being disrupted in many pieces in a close encounter with it. Comets have unstable orbits and they cross the orbits of all the planets, so close encounters can be common. Short period comets have also relatively low inclined orbits, so the the probability of this interaction are greater. They could be responsible for various extinction events, not only because the possibility of an impact with the Earth, but because the possibility of shattering a minor planet like an asteroid that create a new asteroid family, scattering the smallest bodies like bullets through the Solar System. If a comet survives this tragic endings, it could deplete of volatile materials and became an extinct comet, that resemble an asteroid. Damocloids, asteroids with elliptic, comet-like orbits, and many Near Earth Asteroids, like Phaethon, can be extinct comets.
  • Type: Comet.
  • Orbit: Sun.
  • Orbital period: 75.32 yr.
  • Composition: Icy body.
  • Density: 0.6 g/cm3.
  • Dimensions: 15 km × 8 km
  • Model scale: 1:8x104 (20cm) 1:2x105 (8cm)

References

Other astronomical objects

Object

Scale [1:x]

K = 103 (thousand)
M = 106 (million)
G = 109 (billion)

Image

Inner Solar System

Mercury 20M, 60M, 120M image
Venus 60M, 120M, 250M image
Earth 60M, 120M, 250M image
Luna 10M, 20M, 60M image
Mars 20M, 60M, 120M image
Phobos and Deimos 200K, 500K image

Artificial

Salyut 7 40, 48, 80, 160 image

Near Earth Asteroids

Moshup and Squannit 8K, 20K, 40K image
Ra-Shalom 20K, 40K image
Castalia 8K, 20K, 40K image
Bacchus 8K, 20K image
Bennu 3K, 8K image
Ryugu 3K, 8K, 20K image
Geographos 40K, 80K image
Phaethon 40K, 80K image
Itokawa 3K, 8K image
Eros 80K, 200K, 500K image
Nereus 3K, 8K image
Mithra 20K, 40K image
Golevka 8K image
Toutatis 40K, 80K image

Main Asteroid Belt

Gaspra 200K image
Annefrank 40K, 80K image
Braille 20K, 40K image
Vesta 2M, 4M, 10M image
Šteins 40K, 80K, 200K image
Iris 2M, 4M image
Hebe 1M, 2M, 4M image
Lutetia 500K, 1M, 2M image
Julia 1M, 2M, 4M image
Mathilde 500K, 1M image
Juno 2M, 4M image
Ceres 4M, 10M image
Pallas 4M, 10M image
Kleopatra 2M, 4M image
Ida 500K, 1M image
Psyche 2M, 4M image
Interamnia 2M, 4M image
Hygiea 2M, 4M, 10M image
Antiope 1M, 2M image

Jovian System

Jupiter 500M, 1G image
Amalthea 2M, 4M image
Thebe 1M, 2M image
Io 20M, 60M image
Europa 20M, 60M image
Ganymede 60M, 120M image
Callisto 60M, 120M image

Saturn System

Saturn 500M, 1G image
Pan, Daphnis and Atlas 80K, 200K, 500K, 1M image
Prometheus and Pandora 1M, 2M image
Janus and Epimetheus 2M, 4M image
Mimas 2M, 4M, 10M image
Methone, Anthe and Pallene 40K, 80K image
Enceladus 4M, 10M image
Tethys 4M, 10M, 20M image
Telesto and Calypso 200K, 500K image
Dione 4M, 10M, 20M image
Helene 500K, 1M image
Rhea 10M, 20M image
Titan 60M, 120M image
Hyperion 2M, 4M image
Iapetus 10M, 20M image
Phoebe 1M, 2M, 4M image

Uranian System

Uranus 250M, 500M, 1G image
Puck 1M, 2M, 4M image
Miranda 4M, 10M image
Ariel 10M, 20M image
Umbriel 10M, 20M image
Titania 10M, 20M image
Oberon 10M, 20M image

Neptunian System

Neptune 250M, 500M, 1G image
Larissa 2M, 4M image
Proteus 2M, 4M, 10M image
Triton 20M image

Comets

Tempel 1 40K, 80K, 200K image
Wild 2 40K, 80K image
Churyumov-Gerasimenko 20K, 40K, 80K image
Hartley 2 20K, 40K, 80K image
Borrelly 40K, 80K, 200K image
Halley 80K, 200K image

Centaurs and TNOs

Hidalgo 500K, 1M image
Chariklo 2M, 4M image
Pluto and Charon 10M, 20M image
Styx, Nix, Kerberos and Hydra 500K, 1M image
Haumea, Namaka and Hiʻiaka 10M, 20M image
Arrokoth 200K, 500K, 1M image
Largest TNOs and their moons 10M, 20M image

Extrasolar

Exoplanets 120M, 250M, 500M image
Nearest white dwarfs 120M, 250M image
HD 189733 b 1G image
Pulsars 200K, 500K image
Cygnus X-1 accretion disk 10M, 20M image

Sky maps

Heliosphere 7.5*1013, 1.5*1014 image
Constellations - image
CMBR 2*1028 image

Ancient

Earth (540 Mya to 20 Mya) 60M, 120M, 250M image
Luna (4 Gya) 20M, 60M image

Speculative

Planet Nine 250M, 500M image
Cube planet 60M, 120M, 250M image

Science Fiction

Ghroth 4M, 10M image
Arda 60M, 120M image
B612 10, 20, 32, 40 image
Mesklin 500M, 1G image
Arrakis 60M, 120M image
Borg cube 8K, 20K, 40K image
Pern 60M, 120M image
Europa Monolith 200K, 500K image
Leonora Christine 500, 600, 1K, 3K image
Rama 80K, 200K, 500K image
Death Star 500K, 1M, 2M image
Starkiller Base 2M, 4M, 10M image
Nirn, Secunda and Masser 20M, 60M, 120M image
Independence Day mothership 2M, 4M, 10M image
Arrival heptapod spaceship 1K, 3K, 8K image
Gaijin flowership 3K image
Halo Array 4M, 10M, 20M, 60M image
Gem Homeworld 120M, 250M, 500M image
The Skeld 40, 80, 160, 350, 500 image

Misc

Mars (1962 reconstruction) 60M, 120M image
Flat Earth 250M image
Expanding Earth 60M, 120M image
Spaceship of Ezekiel 80, 160 image