Two reasons . . .
1). A larger orbit has a longer distance around it.
2). An object in a larger orbit travels slower. (One of the ways that gravity works.)
Put these two facts together . . .
When you have a longer distance to go, and you move slower,
it's pretty sure that it'll take you longer to finish it.
They are the same
If the further moons have the same velocity as Callisto, they will have longer orbital periods. However, if their velocity is greater, they may have shorter orbital periods.
Synchronous rotation
Johannes Kepler, working with the detailed observational data compiled by Tycho Brahe, showed that the ratio of (orbital period)2 to (mean distance from the sun)3 is a constant for the earth and the five other visible planets. A generation after Kepler, Sir Isaac Newton showed that his law of universal gravitation could predict the shape and periods of the planetary orbits.
When a satelite's rotational period is the same as its orbital period, like our moon, the satelite is tidally locked to the body being orbited. Such a rotation rate is known as a synchronous rotation. The effect is that the same side of the satelite always faces the orbited body.
They are farther away and have larger orbital periods.
They are the same
If the further moons have the same velocity as Callisto, they will have longer orbital periods. However, if their velocity is greater, they may have shorter orbital periods.
The electron cloud increases the amount of valence shells it has with the increase of electrons in the atoms
As you move from left to right on rows, or across periods and top to bottom, or down a group, the number of protons increases.
They all have a filled 1s orbital
Synchronous rotation
Kuiper belt thats all i know
The orbital period depends upon the distance to, and the mass of, the primary. Jupiter, for example, is much more massive than Earth and a correspondingly greater velocity is required to balance out its gravitational pull, meaning that a satellite orbits Jupiter in a much shorter time than it would orbit Earth if it were at the same distance.
it increases. the nuclear charge also increases
Johannes Kepler, working with the detailed observational data compiled by Tycho Brahe, showed that the ratio of (orbital period)2 to (mean distance from the sun)3 is a constant for the earth and the five other visible planets. A generation after Kepler, Sir Isaac Newton showed that his law of universal gravitation could predict the shape and periods of the planetary orbits.
It doesn't orbit earth faster. The ISS is in a lower orbit with a period of 91 minutes compared to the Hubble's orbital period of 96-97 minutes. Orbital periods generally increase with orbit radius and speed in the orbit decreases with increasing orbit radius.