Astrophysics (Index)About

solar system

(the Sun and what's gravitationally bound to it)

The solar system is the Sun plus objects, gas, and dust gravitationally bound to it. (The terms stellar system or star system may be analogously used for stars, but perhaps more often are intended to mean a mean multiple star systems such as a binary stars.) The solar system includes the eight planets, plus dwarf planets, comets, asteroids and similar minor planets/planetoids, including trans-Neptune objects, SSSBs, near-Earth objects, centaurs, plutoids, meteoroids, the Kuiper Belt and Oort Cloud (these are not mutually exclusive categories), the moons of the planets, and the interplanetary medium (IPM). The solar system has proven to be atypical, lacking super-Earths, the most common type of planet in planetary systems, and including gas giants, which are relatively rare.

The history of the solar system is of interest, from planet formation, including Earth's Moon formation, the late heavy bombardment, and planetary migration: eccentricity and orbital inclination of outer planets suggest some migration occurred. Models developed include the Nice model and the grand tack hypothesis. The study of meteorites, many of which are very old, is extremely useful in forming and evaluating the models.


The phrase solar system is also sometimes used for the analogous system around other stars, e.g., TRAPPIST-1's solar system.


(Sun,planets)
Further reading:
https://en.wikipedia.org/wiki/Solar_System
https://en.wikipedia.org/wiki/Star_system
http://hyperphysics.phy-astr.gsu.edu/hbase/Solar/solarcon.html
https://solarviews.com/eng/solarsys.htm
https://pages.uoregon.edu/jschombe/ast121/lectures/lec08.html
https://www.astro.umd.edu/~lgm/ASTR101/ss-facts.html
https://www.physics.unlv.edu/~jeffery/astro/ial/ial_016.html

Referenced by pages:
10199 Chariklo
abundances
ammonia (NH3)
anomalous cosmic rays (ACR)
apsis
asteroid
asteroid belt
astronomical quantities
astronomical unit (AU)
aurora
bathymetry
Birkhoff's theorem
bow shock
C/2014 UN271
CAI
carbon (C)
Carl Sagan Institute (CSI)
Cassini
cavity-enhanced absorption spectroscopy (CEAS)
centaur
chondrite
CMB dipole
collisional erosion
core accretion model
cosmic dust
crustal plates
current sheet
damocloid
debris disk
drogue chute
Earth
Earth analog
earthshine
ecliptic
Einstein delay
energetic neutral atom (ENA)
ephemeris
equatorial coordinate system (EQ)
equilibrium condensation model
equilibrium temperature (Teq)
escape velocity (Ve)
exosatellite
extended source
extra-solar planet
fixed star
Forbush decrease
free-floating planet (FFP)
galactic tide
Ganymede
giant planet
giant star
Gould's Belt
grand tack hypothesis
gravitational instability model
gravitationally bound
gravity assist
greenhouse effect
habitable zone (HZ)
Haumea
heliosphere
helium planet
Hisaki
humidity
hydrocarbon (HC)
Institut de radioastronomie millimétrique (IRAM)
internal gravity wave (IGW)
International Celestial Reference System (ICRS)
interplanetary medium (IPM)
Interstellar Boundary Explorer (IBEX)
intertropical convergence zone (ITCZ)
Io
iron (Fe)
J2
James Clerk Maxwell Telescope (JCMT)
Julian date (JD)
Jupiter
Kelvin-Helmholtz instability (KHI)
Kepler's laws
Lagrangian point
Laplace-Lagrange secular theory
late heavy bombardment (LHB)
Local Bubble
Local Interstellar Cloud (LIC)
long-period comet
Lorentz force
Love number
Lucy
Lyapunov time
M-type star (M)
magnetic field
magnetic induction
Mars
mass extinction
mass spectrometer
Mercury
MERCURY
metallic hydrogen
meteorite
meteoroid
methane (CH4)
Milky Way (MW)
minor planet
modified Newtonian dynamics (MOND)
moon
Moon formation
multi-messenger astronomy (MMA)
NASA
nebular hypothesis
Neptune
New Horizons (NF1)
Nice model
numerical weather prediction (NWP)
obliquity
occultation
occultation observations
oligarch
Oort Cloud
orbital element
orbital inclination
orrery
Other Worlds Laboratory (OWL)
Oumuamua
Outer Solar System Origins Survey (OSSOS)
Pan-STARRS
phase angle
physical field
planet
planet formation
Planet Nine
planet type
planetary differentiation
planetary nebula (PN)
planetary science
planetary system
planetesimal
planetoid
plasma wave
Pluto
polycyclic aromatic hydrocarbon (PAH)
potassium/thorium ratio (K/Th ratio)
presolar grain
primary
provisional designation
quantum system
radar
radiation belt
radioactive dating
retrograde orbit
ring system
ROCKE-3D
Roemer delay
rotating radio transient (RRAT)
rotation period
Saturn
Scholz's Star
Scutum-Centaurus Arm
shell
signatures of formation
snow line
solar day
solar energetic particle (SEP)
solar nebula
solar neighborhood
solar system object (SSO)
solar wind
sounder
SSSB (SB)
star system
strong-field gravity
subsatellite
Sun
Sun surface features
super-Earth
supercritical fluid (SCF)
supernova survey
surface brightness (SB)
SWMF
Terrestrial Time (TT)
theory of figures (TOF)
tidal force
tidal heating
tidal locking
Tillotson equation
time standard
Titan
Titius-Bode law
tomography
TRAPPIST
TXS 0506+056
Uranus
Venus
Voyager
water (H2O)
X-ray flash (XRF)

Index