Unit 2 #2 Flashcards

1
Q

gamma

A

10 to the -12

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

radio waves

A

100 meters

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

frequency

A

write with letter n, number of waves per second, that pass a given point in space

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

x ryas

A

10 to the -10

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

waves

A

Greek letter that is upside down, distance between two consecutive peaks (1 full cycle), light is a wave

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

microwaves

A

10 to the -2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

speed

A

C, speed of the waves, all electro magnetic waves travel at the speed of light

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

infared

A

10 to the -4

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

visbile light

A

in between
4 times 10 to the -7 and ….
7 times 10 to the -7

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

bohr model

A

1.said there is a nucleus and different levels, 2. electrons confined to these levels, 3. when one passes energy through the tube, it takes it to another level and then drops down, 4. electron moves from high level to low levels, in doing so it releases an energy (photon) of light

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

see red light

A

from 1 to 3

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

see green light

A

from 4 then 2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

see blue light

A

from 5 to 2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

energy =….

A

photon’s constant times frequency, can use this to make calculations

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

z

A

atomic number

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

ultraviolent

A

10 to the -8

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

speed of light

A

700 miles per hour

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

electro mangetic radiation

A

includes light, x rays, micro waves, radio waves, all classified based on wave length

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

speed of light

A

wave length (meters) times frequency (1/second)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Rh

A

riburg constant

always 2.178 times 10 to the -18 Joules

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

emission of light by excited hydrogen atoms

A
  1. sample of hydrogen recieve high energy of spark
  2. hydrogen molecule absorb energy and bonds are broken
  3. they then get exicted
  4. they release extra energy by wavelengths to produce emission spectrum of hydrogen atoms
19
Q

continous spectrum

A

white light pass through prism, continas all the wavelengths

20
Q

line spectrum

A

visible region passed through prism only see a few, indicates that only certain energies are alowed for the electron in the hydrogen atom

21
Q

Bohr

A

developed quantum model for the HYDROGEN atom, believed the electron in a hydrogen atom moves around the nucleus only in certain allowed circular orbits, gave hydrogen atom energy levels consistent with the hydrogen emission spectrum

22
the negative in the equation (energy levels available to the electron in the hydrogen atom)
energy of the electron is lower than it would be if the electron were at an infinite distance from the nucleus (interation and energy = zero)
23
ground state
lowest possible energy state
24
the negative in the equation (the change in energy when the electron falls from one level to another
indicates that the atom has lost energy
25
aufbau principle
as protons are added on by one to the nucleus to build up the elements, electrons are simply added to these hydrogenlike orbitals
26
Hund's rule
the lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by Pauli principle in a paritcular set of degenerate orbitals
27
valence electrons
electrons in the outermost principal quantum level of an atom
28
core electrons
inner electrons
29
orbital diagram
ARROWS
30
transition metals
configurations are obtained by adding electrons to the five 3d orbitals
31
important points of the periodic table
1. (n + 1)s orbitals always fill before nd orbitals 2. lanthaninde series or lanthanides (filling of the seven 4f orbitals) 3.actinide series (filling seven 5f orbitals) 4. group label tells the total number of valence electrons for that gro
32
inoization energy
required to remove an electron from a gaseous atom or ion, highest energy electron (one bound least tightly) is removed first
33
first inoization energy
energy required to remove the highest energy of an electron
34
second inoization energy
energy required to removed the second electron
35
when you go to the right....
the first ionization energy increasesoo
36
when you go down a group.....
first innozation decreases (electrons being removed are farther away from the nucleus)
37
electron affinity
energy charge associated with addition of an electron to a gaseous atom (if addition of energy resutls in lower energy, the electron affinity will carry a negative sign)
38
when go left to right (electron affinity)
electron affinity began negative
39
when you go down by group (electron affinity0
electron affinity become positive( (less energy released)
40
atomic radius
atom size cannot specify exactly
41
values for atomic radii
obtained distance between atoms in chemical compounds
42
when left to right (raddi)
atomic radii decreases, valence electrons become closer, decreasing in size
43
when go down a group (radii)
atomic radii increaes
44
metals
left side, cations (give up electrons, become postivie)
45
nometals
right side, gain electrons form anions (negative)
46
metalloids
have metal and nonmetal properties
47
alkali metals
group 1A, going down (first inozation energy decreases, radii increaes), very reactive, low inoziation energy