ILC class h

ILC developing version
Expanded class h

▽ ⌕ `h`	celestial objects; heavenly bodies; cosmic structures; astronomical objects [astronomy; astrophysics; cosmology] ← `g` bulk matter ≈ DDC `520 523` ✍
▽ ⌕ `h09e`	geocentrism; Ptolemaic system
▽ ⌕ `h09eBc`	classical planets ← `hp` planets
▽ ⌕ `h09h`	heliocentrism; Copernican system
▽ ⌕ `h28` `[j8]`	at declination; dec; δ
▽ ⌕ `h282` `[an]`	at ly distance from Earth light years
▽ ⌕ `h282tqto` ⋄	2.50 M ✍
▽ ⌕ `h287` `[j89]`	hour angle; HA; LHA
▽ ⌕ `h288` `[j189]`	at right ascension; RA; α
▽ ⌕ `h288bsrzq` ⋄	0h 42m 44s ✍
▽ ⌕ `h28fsl` ⋄	+41° 16' ✍
▽ ⌕ `h5`	motion [kinematics]
▽ ⌕ `h52` `[an]`	orbiting in terrestrial days revolution period
▽ ⌕ `h526` `[an]`	rotating in terrestrial days rotation period
▽ ⌕ `h585` `[an]`	velocity m/s²; v; speed
▽ ⌕ `h5852` `[j7]`	velocity direction
▽ ⌕ `h5855` `[an]`	acceleration m/s²; a
▽ ⌕ `h5855b`	deceleration; slow down
▽ ⌕ `h5855c`	steady speed
▽ ⌕ `h585c`	still; stationary
▽ ⌕ `h5b`	linear motion; rectilinear motion
▽ ⌕ `h5c`	circular motion ← `cccc` 15 to 30 degrees
▽ ⌕ `h5h`	simple harmonic motion; pendulum
▽ ⌕ `h5o`	orbiting [celestial mechanics]
▽ ⌕ `h5r`	rotating spin
▽ ⌕ `h68` `[g6]`	colour
▽ ⌕ `h7`	structural layer
▽ ⌕ `h70` ⋄	composed of substance
▽ ⌕ `h70ebb` ⋄	hydrogen
▽ ⌕ `h7c`	core
▽ ⌕ `h7m`	middle
▽ ⌕ `h7r`	external layer
▽ ⌕ `h7s`	surface
▽ ⌕ `h7t`	atmosphere
▽ ⌕ `h83` `[an]`	absolute magnitude; M_v
▽ ⌕ `h836` `[an]`	apparent magnitude; m; vmag
▽ ⌕ `h836bmlg` ⋄	-27; Sun apparent magnitude
▽ ⌕ `h84` `[an]`	color index; B-V index; temperature
▽ ⌕ `h84mgfg` ⋄	0.656; Sun B-V index
▽ ⌕ `h9` `[X]`	body kind
▽ ⌕ `h91` `[519]`	evolutionary stage
▽ ⌕ `h91n`	young
▽ ⌕ `h92` `[h]`	orbiting central object
▽ ⌕ `hU`	the Earth ← `hpU` solar planets ≈ DDC `525`
▽ ⌕ `hU7`	Earth structural layer ← `hpt` terrestrial planets
▽ ⌕ `hU7c`	core
▽ ⌕ `hU7cCi`	inner core
▽ ⌕ `hU7cCo`	outer core
▽ ⌕ `hU7m`	mantle
▽ ⌕ `hU7mCe`	lower mantle
▽ ⌕ `hU7mCi`	asthenosphere
▽ ⌕ `hU7mCuWr`	lithosphere
▽ ⌕ `hU7mCu`	upper mantle; lithospheric mantle
▽ ⌕ `hU7mCx`	Moho; Mohorovičić discontinuity
▽ ⌕ `hU7r`	crust ← `i` rocks
▽ ⌕ `hU7rCc`	continental crust; sial
▽ ⌕ `hU7rCo`	oceanic crust; sima
▽ ⌕ `hU7s`	surface
▽ ⌕ `hU7t`	atmosphere
▽ ⌕ `hU7tCb`	troposphere
▽ ⌕ `hU7tCe`	stratosphere
▽ ⌕ `hU7tCm`	mesosphere
▽ ⌕ `hU7tCt`	thermosphere
▽ ⌕ `hU7tCx`	exosphere
▽ ⌕ `hb`	nebulae
▽ ⌕ `hc`	clouds; diffuse nebulae
▽ ⌕ `hce`	molecular clouds
▽ ⌕ `hcg`	Bok globules; Thackeray's globules
▽ ⌕ `hd`	dark matter
▽ ⌕ `hg`	galaxies
▽ ⌕ `hgU`	the Milky Way
▽ ⌕ `hgd`	dwarf galaxies
▽ ⌕ `hge`	elliptical galaxies
▽ ⌕ `hges`	shell galaxies
▽ ⌕ `hgl`	lenticular galaxies
▽ ⌕ `hgp`	spiral galaxies; disk galaxies
▽ ⌕ `hgpb`	barred spiral galaxies
▽ ⌕ `hgr`	ring galaxies
▽ ⌕ `hgt`	irregular galaxies
▽ ⌕ `hgu`	ultra diffuse galaxies; UDGs
▽ ⌕ `hh`	galaxy associations
▽ ⌕ `hhg`	galaxy groups
▽ ⌕ `hhl`	galaxy clusters ✍
▽ ⌕ `hhs`	galaxy superclusters
▽ ⌕ `hk`	brown dwarves
▽ ⌕ `hl`	stars ← `gf` plasma ✍
▽ ⌕ `hl5C`	star process
▽ ⌕ `hl5Cn`	stellar nucleosynthesis
▽ ⌕ `hl9`	spectral type
▽ ⌕ `hl91`	star evolutionary stage
▽ ⌕ `hl91k`	protostars
▽ ⌕ `hl91n`	young stellar objects
▽ ⌕ `hl91p`	main sequence stars
▽ ⌕ `hl91q`	neutron stars
▽ ⌕ `hl9b`	O; blue
▽ ⌕ `hl9c`	B; blue white
▽ ⌕ `hl9e`	A; white
▽ ⌕ `hl9f`	F; yellow white
▽ ⌕ `hl9g`	G; yellow
▽ ⌕ `hl9k`	K; orange
▽ ⌕ `hl9m`	M; red
▽ ⌕ `hl9r`	L
▽ ⌕ `hl9t`	T
▽ ⌕ `hlU`	the Sun ← `hld` dwarf stars `hl91n` young stellar objects
▽ ⌕ `hlb`	subdwarf stars
▽ ⌕ `hld`	dwarf stars
▽ ⌕ `hlf`	subgiant stars
▽ ⌕ `hlg`	giant stars
▽ ⌕ `hlh`	bright giant stars
▽ ⌕ `hlj`	supergiant stars
▽ ⌕ `hlk`	hypergiant stars
▽ ⌕ `hp`	planets [planetary science] ✍
▽ ⌕ `hpU`	solar planets ← `hlU` the Sun
▽ ⌕ `hpUc`	Mercury
▽ ⌕ `hpUe`	Venus
▽ ⌕ `hpUm`	Mars
▽ ⌕ `hpUp`	Jupiter
▽ ⌕ `hpUs`	Saturn
▽ ⌕ `hpUu`	Uranus
▽ ⌕ `hpUw`	Neptune
▽ ⌕ `hpg`	giant planets
▽ ⌕ `hpt`	terrestrial planets; telluric; rocky planets
▽ ⌕ `hpt7s`	surface
▽ ⌕ `hpt7t`	atmosphere
▽ ⌕ `hq`	minor planets; planetoids
▽ ⌕ `hqd`	dwarf planets
▽ ⌕ `hqdU`	solar dwarf planets ← `hlU` the Sun
▽ ⌕ `hqdUc`	Ceres
▽ ⌕ `hqdUp`	Pluto
▽ ⌕ `hqf`	asteroids
▽ ⌕ `hqj`	trojans
▽ ⌕ `hqn`	centaurs ← `hlU` the Sun
▽ ⌕ `hr`	meteoroids; meteors
▽ ⌕ `hs`	planetary satellites; natural satellites; moons
▽ ⌕ `hs92pUp` ⋄	Jupiter satellites
▽ ⌕ `hsU`	the Moon
▽ ⌕ `ht`	planetary systems; star systems; stellar systems
▽ ⌕ `htU`	the Solar system ← `hlU` the Sun
▽ ⌕ `htUat`	comets
▽ ⌕ `htc`	binary stars
▽ ⌕ `htd`	triple star systems
▽ ⌕ `hu`	star clusters; stellar clusters ← `hl` stars
▽ ⌕ `huU`	Pleiades
▽ ⌕ `hug`	globular clusters; GCs
▽ ⌕ `hui`	intermediate star clusters
▽ ⌕ `huo`	open clusters
Connected classes:
`g388` `[h5]`	potential energy; motion
`h09eBc`	classical planets ← `hp`
`h92` `[h]`	orbiting central object
`hU`	the Earth ← `hpU`
`hU7`	Earth structural layer ← `hpt`
`hlU`	the Sun ← `hld hl91n`
`hpU`	solar planets ← `hlU`
`hqdU`	solar dwarf planets ← `hlU`
`hqn`	centaurs ← `hlU`
`htU`	the Solar system ← `hlU`
`hu`	star clusters; stellar clusters ← `hl`
`i31` `[hU7]`	from structural layer
`it`	tectonic plates [plate tectonics] ← `hUal`
`itt`	plates of the Earth ← `hU`
`j28` `[hp]`	on planet
`j3`	weather [meteorology] ← `hUap`
`j5b`	impact events ← `hqf`
`jU`	landmasses of the contemporary Earth; continents, microcontinents ← `js hU`
`jdU`	mountain ranges of contemporary Earth ← `hU`
`jyU`	seas of the contemporary Earth; World Ocean ← `hU`
`n5m234`	migrating towards ← `h5`
`r3v`	solar power; solar energy ← `hlU`
`svr`	aircrafts ← `hU7t`
`woih`	horoscopes; natal charts; celestial maps; cosmograms; vitaspheres; radical charts [astrology] ← `h`
`wrn`	naturalism ← `g h i j k l m`
`ygh`	astronomy ← `h`

specificity
current: 99

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ILC developing version — ISKO Italia <https://www.iskoi.org/ilc/> : 2006.03.06 - 2026.05.14 -

ILC developing versionExpanded class h

ILC developing version
Expanded class `h`