New Study Method Flashcards

1
Q

Newton’s 1st Law

A

Objects resist change in motion (inertia).

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2
Q

Newton’s 2nd Law

A

Force = mass x accleration
f=ma

Acceleration happens when a net force is applied.

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3
Q

Newton’s 3rd Law

A

Equal & opposite forces (action-reaction).

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4
Q

When does Newton’s 2nd Law NOT apply?

A

At constant speed, acceleration = 0.

Remember:
No acceleration →
No net force →
Newton’s 2nd Law (F = ma) does NOT apply

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5
Q

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

A

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.
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6
Q

Why Do Planets Orbit in the Same Direction?

A

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

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7
Q

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

A

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

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8
Q

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

A

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.

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9
Q

What do small stars become after they die?

A

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

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10
Q

What determines an element’s identity?

A

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

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11
Q

What are the major trends on the periodic table?

A

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.

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12
Q

How do electron orbitals determine stability?

A

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.

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13
Q

How do you write electron configurations?

A

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).

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