Reading · Listening

TOEFL Astronomy & Physics Vocabulary

Astronomy and physics passages frequently appear on the TOEFL Reading section, often discussing planetary formation, stellar life cycles, or fundamental physical principles. The vocabulary below covers the core concepts — celestial bodies, motion, energy, and observation — that recur across these passages.

Word Definition & Example
galaxy
n.
A massive system of stars, gas, and dust held together by gravity.
"The Milky Way galaxy contains roughly 200 billion stars."
Collocations: spiral galaxy, distant galaxy
orbit
n. / v.
The curved path of an object around a star, planet, or moon.
"The Moon orbits Earth approximately once every 27 days."
Collocations: stable orbit, orbital period
gravity
n.
The force that attracts objects with mass toward each other.
"Gravity holds planets in their orbits around the Sun."
Collocations: force of gravity, gravitational pull
mass
n.
The amount of matter in an object.
"Jupiter has more mass than all the other planets combined."
Collocations: atomic mass, total mass
density
n.
Mass per unit volume.
"Saturn has such low density that it would float in water."
Collocations: high density, density of a substance
radiation
n.
Energy that travels in the form of waves or particles.
"Solar radiation reaches Earth in just over eight minutes."
Collocations: electromagnetic radiation, harmful radiation
spectrum
n.
The range of colours or wavelengths into which light can be separated.
"By analysing a star's spectrum, astronomers determine its composition."
Collocations: electromagnetic spectrum, visible spectrum
wavelength
n.
The distance between two corresponding points of a wave.
"Red light has a longer wavelength than blue light."
Collocations: long wavelength, short wavelength
nebula
n.
A vast cloud of gas and dust in space.
"Stars are born inside stellar nebulae."
Collocations: stellar nebula, planetary nebula
supernova
n.
A massive stellar explosion at the end of a star's life.
"A supernova outshines an entire galaxy for several weeks."
Collocations: supernova explosion
asteroid
n.
A small rocky body orbiting the Sun.
"The asteroid belt lies between Mars and Jupiter."
Collocations: asteroid belt, Near-Earth asteroid
comet
n.
An icy body that releases gas as it approaches the Sun.
"Halley's Comet returns to view from Earth roughly every 76 years."
Collocations: comet's tail
telescope
n.
An instrument used to observe distant objects.
"The Hubble telescope orbits Earth above the atmosphere."
Collocations: optical telescope, radio telescope
constellation
n.
A group of stars forming a recognisable pattern.
"Orion is one of the most easily identified constellations."
Collocations: winter constellation
light-year
n.
The distance light travels in one year — about 9.5 trillion kilometres.
"Proxima Centauri is 4.2 light-years from Earth."
Collocations: many light-years away
velocity
n.
Speed in a particular direction.
"The space shuttle reached an orbital velocity of about 28,000 km/h."
Collocations: high velocity, terminal velocity
acceleration
n.
The rate at which velocity changes.
"Earth's gravitational acceleration is approximately 9.8 m/s²."
Collocations: constant acceleration
energy
n.
The capacity to do work or produce heat.
"The Sun radiates an enormous amount of energy in all directions."
Collocations: kinetic energy, potential energy
particle
n.
An extremely small piece of matter.
"Electrons are subatomic particles with a negative charge."
Collocations: subatomic particle, charged particle
solar system
n.
The Sun together with all the bodies that orbit it.
"Our solar system formed about 4.6 billion years ago."
Collocations: outer solar system
atmosphere
n.
The layer of gases surrounding a planet or star.
"Venus has a dense atmosphere of carbon dioxide."
Collocations: thin atmosphere, planetary atmosphere
eclipse
n.
An event where one celestial body blocks light from another.
"A lunar eclipse occurs when Earth's shadow falls on the Moon."
Collocations: solar eclipse, lunar eclipse
fusion
n.
The combining of atomic nuclei to release energy.
"Nuclear fusion powers the Sun and other stars."
Collocations: nuclear fusion, fusion reactor
expand
v.
To increase in size or volume.
"Astronomical observations show that the universe is expanding."
Collocations: expand rapidly
observe
v.
To watch carefully in order to gather information.
"Galileo was the first to observe the moons of Jupiter through a telescope."
Collocations: observe a phenomenon

How this vocabulary appears on the TOEFL

Astronomy & Physics terms appear directly in passages and audio across Reading · Listening. The questions you'll see most frequently target this vocabulary are paraphrase identification (the test rewords a sentence using a synonym from this list), inference questions (you need the term's meaning to follow the argument), and reference questions (the term is the antecedent of a pronoun in another sentence). Knowing the term plus one or two natural collocations lets you decode passages faster and recognise paraphrases on the answer choices without re-reading.

How to study this list effectively

Don't try to memorise the whole list in one sitting. Effective vocabulary study works in three passes: (1) recognise — read each entry once until the word feels familiar; (2) retrieve — cover the definitions and try to recall each one from the word alone; (3) produce — write a sentence of your own that uses the word in a TOEFL context. Spaced repetition over 5–7 days will make the words stick far better than a single intensive review session. Pair this list with a practice test in the same section so you encounter the words in real test contexts.

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