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The orbital speed would be approximately 7.63 km/s and the period would be approximately 95.59 minutes for a satellite orbiting Earth at an altitude of 1.44 x 10^3 m. These values can be calculated using the formula for orbital speed (v = √(GM/r)) and the formula for orbital period (T = 2π√(r^3/GM)), where G is the gravitational constant, M is the mass of Earth, and r is the altitude of the satellite above Earth's surface.
It depends whether you mean ml or ms.There are 4 quantum numbers, n, l, ml, msThey have long names respectively principal, azimuthal (angular momentum), magnetic and spin.n can have values 0, 1, 2, 3, 4, 5......l depends on n, and can have values, 0 to (n-1) (0 is an s orbital, 1 is a p subshell, 2 is a d subshell, 3 is a f subshell etcml can have -l to +l (sorry this font is rubbish the letter l looks like a 1) so for a d orbital, where l = 2, it can be -2, -1 0, +1, +2. Five d orbitals in all.ms can be -1/2 or +1/2 (These are the maximum of 2 electrons having opposite spin)l depends on n, and can have values, 0 to (n-1) (0 is an s orbital, 1 is a p subshell, 2 is a d subshell, 3 is a f subshell etcRead more: What_are_the_possible_values_for_the_quantum_numbers
You can use the formula M = (V^2 * R) / G, where M is the planet's mass, V is the orbital speed, R is the distance from the sun, and G is the gravitational constant. By plugging in the values of V and R, you can calculate the planet's mass.
A low-lying sigma molecular orbital is a symmetrical orbital formed by the overlap of atomic orbitals in a molecule. It typically has a relatively low energy level compared to other molecular orbitals, and it plays a key role in bonding between atoms in a molecule. The "m" designation in this context may refer to a molecular orbital belonging to a specific symmetry group in molecular orbital theory.
The third quantum number, m, describes the orientation of the atomic orbital in space. It specifies the orientation of the orbital within a particular subshell. The values of m range from -l to +l, where l is the azimuthal quantum number.
The specific orbital within a
To calculate the orbital period of a planet, you can use Kepler's third law of planetary motion. The formula is T2 (42 r3) / (G M), where T is the orbital period, r is the average distance from the planet to the sun, G is the gravitational constant, and M is the mass of the sun. Simply plug in the values for r and M to find the orbital period of the planet.
The third quantum number for a 2p3 electron in phosphorus is the magnetic quantum number (m). It specifies the orientation of the orbital in space and can have values ranging from -l to +l, where l is the azimuthal quantum number for the orbital. So, for the 2p orbital with l=1, the possible values of m are -1, 0, and 1.
For the d orbital, the value of l is 2 and the value of ml is - l to + l, so the values of ml would be -2, -1, 0, +1, +2. So, the maximum value would be +2.
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An atomic orbital is a mathematical term signifying the characteristics of the 'orbit' or cloud created by movement of an electron or pair of electrons within an atom. Angular momentum, signified as l, defines the angular momentum of the orbital's path as opposed to values n and m which correspond with the orbital's energy and angular direction, respectively.
nl;m
m(I)=0 (apex)
The orbital speed would be approximately 7.63 km/s and the period would be approximately 95.59 minutes for a satellite orbiting Earth at an altitude of 1.44 x 10^3 m. These values can be calculated using the formula for orbital speed (v = √(GM/r)) and the formula for orbital period (T = 2π√(r^3/GM)), where G is the gravitational constant, M is the mass of Earth, and r is the altitude of the satellite above Earth's surface.
It depends whether you mean ml or ms.There are 4 quantum numbers, n, l, ml, msThey have long names respectively principal, azimuthal (angular momentum), magnetic and spin.n can have values 0, 1, 2, 3, 4, 5......l depends on n, and can have values, 0 to (n-1) (0 is an s orbital, 1 is a p subshell, 2 is a d subshell, 3 is a f subshell etcml can have -l to +l (sorry this font is rubbish the letter l looks like a 1) so for a d orbital, where l = 2, it can be -2, -1 0, +1, +2. Five d orbitals in all.ms can be -1/2 or +1/2 (These are the maximum of 2 electrons having opposite spin)l depends on n, and can have values, 0 to (n-1) (0 is an s orbital, 1 is a p subshell, 2 is a d subshell, 3 is a f subshell etcRead more: What_are_the_possible_values_for_the_quantum_numbers
The equation for orbital velocity is (v = \sqrt{\frac{GM}{r}}), where (v) is the orbital velocity, (G) is the gravitational constant, (M) is the mass of the central body, and (r) is the distance from the center of mass.