Back to marketplace

New Study Method

No description yet. This curated deck is ready for daily study.

Total cards: 13•Content version: v4•Public deck•Updated: 8/1/2026

Card preview (13)

#1
Front (Question)

Newton’s 1st Law

Back (Answer)

Objects resist change in motion (inertia).

#2
Front (Question)

Newton’s 2nd Law

Back (Answer)

Force = mass x accleration f=ma Acceleration happens when a net force is applied.

#3
Front (Question)

Newton’s 3rd Law

Back (Answer)

Equal & opposite forces (action-reaction).

#4
Front (Question)

When does Newton’s 2nd Law NOT apply?

Back (Answer)

At constant speed, acceleration = 0. Remember: No acceleration → No net force → Newton’s 2nd Law (F = ma) does NOT apply

#5
Front (Question)

Why Do Objects Stay in Orbit Instead of Falling into the Sun?

Back (Answer)

Planets and other objects stay in orbit because of a balance between their speed and the Sun’s gravitational pull. • If a planet slows down too much, gravity pulls it in, and it spirals toward the Sun. • If a planet moves too fast, gravity can’t hold it, and it escapes into space.

#6
Front (Question)

Why Do Planets Orbit in the Same Direction?

Back (Answer)

Early planets moved randomly, but gravity & collisions removed unstable ones, leaving only the same-direction orbits.

#7
Front (Question)

What process powers a star, and what does it do?

Back (Answer)

Nuclear Fusion hydrogen atoms fuse into helium, releasing energy that powers the star.

#8
Front (Question)

What happens when a star’s core turns into iron?

Back (Answer)

When a star’s core turns to iron, it can’t make energy anymore. Gravity pulls everything inward, the core collapses, and the star explodes as a supernova.

#9
Front (Question)

What do small stars become after they die?

Back (Answer)

Small stars shrink into white dwarfs, which slowly cool over time into black dwarfs.

#10
Front (Question)

What determines an element’s identity?

Back (Answer)

The number of protons in an atom’s nucleus. However, the number of neutrons can vary (isotopes), but protons never change.

#11
Front (Question)

What are the major trends on the periodic table?

Back (Answer)

Elements follow patterns based on atomic structure and reactivity. Left side = Metals (lose electrons easily, good conductors). Right side = Nonmetals (gain/share electrons, poor conductors). Noble gases (far right) = Unreactive because they have full valence shells. Alkali metals (far left) = Super reactive, want to lose 1 electron. Halogens (second to last column) = Highly reactive, want to gain 1 electron.

#12
Front (Question)

How do electron orbitals determine stability?

Back (Answer)

Electrons fill s, p, and d orbitals in energy levels, impacting reactivity. s-orbital = Holds 2 electrons. p-orbital = Holds 6 electrons → Together, s + p = stable octet (8 total). d-orbital = Holds 10 electrons but doesn’t always need to be full.

#13
Front (Question)

How do you write electron configurations?

Back (Answer)

se the format (shell number) (orbital letter) (electron count) to show how electrons fill orbitals. Example: Carbon (C) = 1s² 2s² 2p² s-orbital holds 2, p-orbital holds 6, d-orbital holds 10. Elements “want” full outer shells (octet rule = 8 valence electrons). Shortcut: Use noble gas notation (e.g., [Ne] 3s² for Mg).