DSST Astronomy study materials
DSST Astronomy study resources

DSST Astronomy cheat sheet

DSST Astronomy · Keep the key ideas within reach.

Quick reference

Celestial Mechanics

  • Kepler's first law: planetary orbits are ellipses with the Sun at one focus; eccentricity e = c/a, where c is the focal distance from center and a is the semimajor axis.

  • Kepler's second law: a line from Sun to planet sweeps equal areas in equal times; orbital speed is greatest at perihelion and least at aphelion.

  • Kepler's third law: P^2 = a^3 when P is in years and a is in astronomical units (AU); more generally P^2 = 4π^2 a^3 / [G(M + m)].

  • Newton's law of gravitation: F = G m1 m2 / r^2, with G = 6.674×10^-11 N·m^2/kg^2; the force is attractive and acts along the line joining the centers.

  • Circular orbital speed: v = sqrt(GM/r); escape speed from a body of mass M and radius R is v_esc = sqrt(2GM/R) = sqrt(2) × v_circular at that radius.

  • Newton's form of Kepler's third law for the solar system: P^2 = a^3 / (M_total in solar masses); for binary stars, total mass M1 + M2 = a^3 / P^2 in solar units.

  • Tidal force scales as 1/r^3; differential gravity stretches a body along the line to the primary and compresses it perpendicular to that line.

  • Conservation laws: angular momentum L = m v r sin θ is constant in a central force field; orbital energy E = 1/2 m v^2 − GMm/r is constant, with E < 0 for bound orbits.

  • Roche limit: a satellite held together only by gravity is torn apart inside roughly 2.44 R_primary (density ratio)^(1/3); this explains ring systems.

Quick reference

Celestial Systems

  • Hierarchy of structure: planet–moon systems, star clusters, galaxies, galaxy groups and clusters, superclusters, and the cosmic web of filaments and voids.

  • Open clusters: young (10^7–10^9 yr), metal-rich, irregular, found in galactic disks, contain 10^2–10^3 stars; example: Pleiades.

  • Globular clusters: old (10^10 yr), metal-poor, spherical, orbit galactic halos, contain 10^5–10^6 stars; example: Omega Centauri.

  • Eclipsing binaries: orbital plane nearly edge-on to Earth; light curves yield radii and, combined with radial velocities, stellar masses.

  • Spectroscopic binaries: detected through periodic Doppler shifts of spectral lines; double-lined systems give mass ratio directly.

  • Visual binaries: resolvable as two stars; Kepler's third law applied to the relative orbit gives total mass.

  • Star clusters are used as cosmic laboratories because member stars share age and initial composition, producing clean Hertzsprung–Russell diagrams.

  • The Local Group contains the Milky Way, Andromeda (M31), Triangulum (M33), and dozens of dwarf galaxies; diameter roughly 3 Mpc.

  • Galaxy clusters contain hundreds to thousands of galaxies, hot intracluster gas (10^7–10^8 K, X-ray emitting), and dark matter; example: Coma Cluster.

Quick reference

Astronomical Instruments

  • Refracting telescope: objective lens; chromatic aberration limits aperture; practical maximum aperture about 1 m.

  • Reflecting telescope: concave primary mirror; no chromatic aberration; examples: Newtonian, Cassegrain, Ritchey–Chrétien.

  • Angular resolution (Rayleigh criterion): θ = 1.22 λ / D radians; larger aperture D or shorter wavelength λ gives finer resolution.

  • Light-gathering power scales as D^2; a 200 mm telescope collects 4 times the light of a 100 mm telescope.

  • Magnification = focal length of objective / focal length of eyepiece; useful magnification is limited by atmospheric seeing and aperture.

  • CCD detectors replaced photographic plates; quantum efficiency can exceed 80% versus a few percent for film.

  • Spectrographs disperse light with prisms or diffraction gratings; gratings give higher dispersion and linear wavelength calibration.

  • Radio telescopes need large dishes for resolution; interferometry (VLBI) combines widely separated antennas to synthesize an aperture equal to the baseline.

  • Adaptive optics uses a deformable mirror and a wavefront sensor (often a laser guide star) to correct atmospheric turbulence in real time.

Quick reference

The Solar System

  • Terrestrial planets: Mercury, Venus, Earth, Mars - small, rocky, high density, few or no moons, no ring systems.

  • Jovian planets: Jupiter, Saturn, Uranus, Neptune - large, low density, hydrogen/helium rich, many moons, ring systems.

  • Asteroid belt lies between Mars and Jupiter at 2.2–3.3 AU; Kuiper Belt lies beyond Neptune at about 30–50 AU.

  • Nebular hypothesis: solar system formed from a collapsing rotating cloud; conservation of angular momentum produced a flattened disk, and planetesimals accreted from dust.

  • Solar composition by mass: about 71% hydrogen, 27% helium, 2% heavier elements; energy from core hydrogen fusion via the proton–proton chain.

  • Sun's core temperature about 15 million K; photosphere about 5,800 K; sunspots are cooler regions (~4,000 K) tied to magnetic activity.

  • Venus has a runaway greenhouse effect: surface temperature about 730 K, atmospheric pressure about 90 times Earth's, dominated by CO2 and sulfuric acid clouds.

  • Mars shows evidence of past liquid water (valley networks, layered sediments); present atmosphere is thin CO2, about 0.6% of Earth's pressure.

  • Jupiter's Great Red Spot is a long-lived anticyclonic storm; Jupiter has four large Galilean moons: Io (volcanic), Europa (ice ocean), Ganymede (largest moon), Callisto.

Quick reference

Nature & Evolution of Stars

  • Spectral classes in order of decreasing temperature: O, B, A, F, G, K, M; the Sun is G2.

  • Hertzsprung–Russell diagram plots luminosity versus temperature (or spectral class); main sequence runs diagonally from hot, luminous O stars to cool, dim M stars.

  • Mass–luminosity relation for main-sequence stars: L/L_sun ≈ (M/M_sun)^3.5; more massive stars are far more luminous and shorter-lived.

  • Stellar structure balance: hydrostatic equilibrium (pressure gradient vs. gravity) and thermal equilibrium (energy generation vs. radiation).

  • Energy generation: proton–proton chain dominates in stars like the Sun; CNO cycle dominates in stars more massive than about 1.3 M_sun.

  • Main-sequence lifetime: t ≈ 10^10 (M/M_sun)^−2.5 years; a 10 M_sun star lives roughly 3×10^7 years.

  • Low-mass stars end as white dwarfs (supported by electron degeneracy pressure), possibly after a planetary-nebula phase.

  • High-mass stars end as core-collapse supernovae (Type II), leaving neutron stars or black holes; Type Ia supernovae come from white dwarfs in binary systems.

  • Stellar remnants: white dwarf mass limit about 1.4 M_sun (Chandrasekhar); neutron star mass limit about 2–3 M_sun; black hole Schwarzschild radius R_s = 2GM/c^2.

Quick reference

The Galaxy

  • Milky Way is a barred spiral galaxy; diameter about 100,000 light-years; the Sun lies about 26,000 light-years from the center.

  • Galactic components: thin disk (young stars, gas, dust), thick disk, central bulge, and stellar halo with globular clusters.

  • Differential rotation: inner regions orbit faster than outer regions; the rotation curve is measured via 21 cm hydrogen emission and stays roughly flat at large radii, implying dark matter.

  • Sun's orbital speed around the galaxy is about 220 km/s; one galactic year is roughly 230 million years.

  • Interstellar medium phases: molecular clouds (cold, dense, star-forming), neutral hydrogen (H I), ionized H II regions, and hot coronal gas.

  • Dust extinction reddens starlight because shorter wavelengths scatter more; observed color must be corrected for interstellar reddening.

  • Spiral arms are density waves, not fixed material; star formation concentrates in arms where gas clouds are compressed.

  • Galactic center hosts the radio source Sagittarius A*, a supermassive black hole of about 4 million solar masses.

  • Population I stars are young, metal-rich, disk stars; Population II stars are old, metal-poor, halo and globular-cluster stars.

Quick reference

The Universe

  • Hubble's law: v = H0 × d, with H0 about 70 km/s/Mpc; recession velocity is proportional to distance for galaxies beyond the Local Group.

  • Cosmological redshift: z = (λ_observed − λ_emitted)/λ_emitted; for small z, v ≈ c z.

  • Big Bang evidence: cosmic microwave background (T ≈ 2.725 K), primordial light-element abundances, and observed galaxy recession.

  • CMB was emitted at recombination (z ≈ 1,100, about 380,000 years after the Big Bang) when the universe became transparent.

  • Friedmann equation governs expansion: H^2 = (8πG/3)ρ − k c^2/a^2 + Λc^2/3; critical density ρ_c = 3H0^2/(8πG).

  • Density parameter Ω = ρ/ρ_c; Ω_total = 1 corresponds to a flat universe; current measurements give Ω_matter ≈ 0.3 and Ω_Λ ≈ 0.7.

  • Dark energy drives accelerated expansion; the accelerating phase began when the universe was several billion years old.

  • Nucleosynthesis in the first few minutes produced about 75% hydrogen and 25% helium by mass, plus trace deuterium and lithium.

  • Age of the universe from current cosmological parameters is about 13.8 billion years.

Quick reference

Determining Astronomical Distances

  • Parallax: p (arcseconds) = 1 / d (parsecs); a star at 1 pc has a parallax of 1 arcsecond; 1 pc = 3.26 light-years = 3.086×10^16 m.

  • Stellar parallax is limited by atmospheric seeing and spacecraft precision; Gaia measures parallaxes to microarcsecond levels for bright stars.

  • Standard candles: objects of known intrinsic luminosity L; apparent brightness b = L / (4π d^2), so d = sqrt(L / 4π b).

  • Distance modulus: m − M = 5 log10(d) − 5, with d in parsecs; m is apparent magnitude, M is absolute magnitude.

  • Cepheid variables follow a period–luminosity relation; longer periods mean greater luminosity, enabling distance measurement in nearby galaxies.

  • Type Ia supernovae are standardizable candles visible at cosmological distances; they revealed accelerated expansion.

  • Tully–Fisher relation uses galaxy rotation width versus luminosity for spiral galaxies; Faber–Jackson uses velocity dispersion versus luminosity for ellipticals.

  • Redshift-based distances require a cosmological model; Hubble's law is reliable only for large-scale distances where peculiar velocities are small.

  • Magnitude scale: a difference of 5 magnitudes equals a brightness ratio of 100; each magnitude is a factor of about 2.512.

Quick reference

Life in the Universe

  • Habitable zone: range of orbital distances where liquid water can exist on a planet's surface; location depends on stellar luminosity and spectral type.

  • Drake equation: N = R* × f_p × n_e × f_l × f_i × f_c × L; estimates of N span many orders of magnitude because several factors are poorly constrained.

  • SETI searches for narrow-band radio signals (for example, the 21 cm hydrogen line) and optical laser pulses; no confirmed extraterrestrial signal has been detected.

  • Fermi paradox: given the age and size of the galaxy, if intelligent life were common we would expect evidence of it; proposed resolutions include rare-Earth hypotheses and short civilization lifetimes.

  • Extremophiles on Earth (thermophiles, halophiles, psychrophiles) expand the range of conditions considered potentially habitable.

  • Biosignatures include atmospheric oxygen and ozone together, methane in disequilibrium, and spectral features of chlorophyll-like pigments.

  • Mars and icy moons Europa and Enceladus are leading targets in the search for past or present life because of evidence for liquid water.

  • Panspermia proposes that life or its precursors can travel between bodies on meteorites; it does not explain the origin of life itself.

  • Rare-Earth hypothesis argues that complex life requires many unusual conditions, such as a large moon, plate tectonics, and a Jupiter-like planet to reduce impact rates.