00:01
So this video we're gonna talk about question 74 from chapter two, which says, for each of the following atomic numbers used the periodic table to write the formula, including the charge for the simple eye on the element is most likely to form and ionic compounds.
00:17
So in a way, we're given on atomic number of 13.
00:22
So let's look in the periodic table for the moment.
00:25
With an atomic number are 13.
00:28
So the element atomic number 13 is aluminum over here.
00:33
Um, and, uh, it's kind of an exception.
00:37
Most rules, but aluminum usually takes a positive three charge when it becomes an eye on.
00:44
And i think unease e way to remember that is that aluminum, zinc and silver the charges that they usually take when they become ions are plus three plus two in plus one.
00:56
So we have 3 to 1 on this little staircase from aluminum, zinc to silver.
01:01
So +321 is a good way of remembering that, um, so for this one, we have et al three plus, um, and then and b, we want the element with an atomic number of 34.
01:23
So the element with an atomic number of 34 is selenium is over here.
01:30
Um, and how do we know what charge cellini, um, prefers to take when it becomes an eye on, um, well, the most useful thing to think about when you're trying to determine this.
01:41
There are exceptions to this, but in general, are all of the elements want to have the noble gas configuration? it's just the most stable on electronic configuration.
01:54
So they wanna have the school electron shell that corresponds to the electron configuration of these elements.
01:59
It's on the far right column of the periodic table.
02:03
Um, so in order to do that, they either gain or lose electrons.
02:08
So, for example, selenium would gain two electrons in order to have the electronic configuration matching krypton, which would be more stable.
02:19
Um, so cellini was gonna take a minus two charge, but you can see elements that are on the left hand side of the periodic table.
02:27
It would be easier to lose electrons rather than gain them in order to reach the noble gas configuration that's closest to them.
02:35
That's, um, requires adding or removing the fewest number of electrons.
02:41
But anyway, and for b, we have cellini.
02:44
Um, so we have s e.
02:45
And we have a minus two charge.
02:47
So us e to minus, um, and see, we have an atomic number of 56...