For larger orbital radii, the orbital periods increase. This is because the gravitational force decreases with distance, leading to slower speeds and longer times to complete an orbit. Kepler's third law states that the square of the orbital period is proportional to the cube of the semi-major axis length.
It depends on the radius of the orbit. Different orbit radii have different orbital periods. As an example, one of Mars's natural satellites, Phobos takes 7.66 hours to orbit Mars. It's orbital radius is around 9,400 km.
Noble gases have larger atomic radii than alkali metals in the same period.
Inner planets are typically rocky, smaller in size, have shorter orbital periods, and lack rings. Outer planets are gaseous or icy, larger in size, have longer orbital periods, and possess rings and many moons. Additionally, inner planets are closer to the Sun, while outer planets are farther away.
To determine which planet is closest to the Sun based on their orbital periods, we can use Kepler's Third Law, which states that the square of a planet's orbital period is proportional to the cube of its average distance from the Sun. Generally, planets with shorter orbital periods are closer to the Sun. Without the specific values from the table, we cannot identify which planet (A, B, C, or D) is closest, but the one with the shortest orbital period would be the closest to the Sun.
Comets are classified based on the length of their orbital period and their origin. Short-period comets have orbital periods less than 200 years, while long-period comets have longer orbital periods. Comets can also be classified based on their composition and physical characteristics, such as size and brightness.
They are farther away and have larger orbital periods.
It depends on the radius of the orbit. Different orbit radii have different orbital periods. As an example, one of Mars's natural satellites, Phobos takes 7.66 hours to orbit Mars. It's orbital radius is around 9,400 km.
Moons beyond the orbit of Callisto would have larger orbital periods than Callisto because they are farther from Jupiter and will take more time to complete one orbit around the planet. This relationship follows Kepler's Third Law of planetary motion, which states that the orbital period of a moon increases as its distance from the planet it orbits increases.
A solar radii is used to express the comparison from one star to our own Sun. If a star has a radius of 10.3 solar radii, then it has a radius 10.3 times larger than the Sun
The 2s orbital is larger than the 1s orbital and is higher in energy.
In a group of metals, ionic radii tend to increase as you move down the group. This is because the outermost electron shell becomes farther from the nucleus as you move down the group, leading to larger atomic sizes and therefore larger ionic radii.
They all have a filled 1s orbital
Van der Waals radii are larger than atomic radii because they include the space occupied by the electron clouds around the atom, which are not considered in atomic radii. Van der Waals radii are used to estimate the effective size of atoms when they are close to each other and experience van der Waals forces.
the 1s orbital is closer to the nucleus and has a lower energy level compared to the 2s orbital. Additionally, the 2s orbital has a slightly higher energy, larger size, and can hold more electrons than the 1s orbital.
Atomic radii refer to the size of an atom, measured as the distance from the center of the nucleus to the outer electron shell. Ionic radii, on the other hand, refer to the size of an ion, which can be larger (anions) or smaller (cations) than the corresponding atom due to the gain or loss of electrons.
Noble gases have larger atomic radii than alkali metals in the same period.
Inner planets are typically rocky, smaller in size, have shorter orbital periods, and lack rings. Outer planets are gaseous or icy, larger in size, have longer orbital periods, and possess rings and many moons. Additionally, inner planets are closer to the Sun, while outer planets are farther away.