The eight motions of the Earth are rotation, revolution, precession, nutation, axial tilt, orbital inclination, apsidal precession, and proper rotation. These motions contribute to phenomena such as day and night (rotation), changing seasons (axial tilt), and variations in the position of the Earth's axis and orbit over time (precession and apsidal precession).
The shape of Earth's orbit becomes more or less oval (eccentricity), Earth wobbles as it spins (precession), and Earth's axis changes too (tilt).
precession
The natural cause of climate change that deals with changes to Earth's orbit around the Sun is known as Milankovitch cycles. These cycles involve variations in the Earth's orbit, tilt, and precession, which can affect the amount and distribution of solar energy received by the Earth, ultimately influencing climate patterns over long timescales.
Titan's orbit has a tilt of approximately 0.1Ëš
Precession
We're not quite sure what the question means by "earth's tilt" or "stay the same".The axis of the earth's rotation is inclined about 67.5 degrees to the plane ofthe earth's orbit, and that doesn't change. Over the course of a human lifetime,or several human lifetimes, the pole of earth's axis remains pointed toward thesame spot in the sky, presently quite close to the star Polaris. Over a period of26,000 years, the pole describes a circle in the sky, but the axis remain inclinedto the plane of the orbit by the same 67.5 degrees.So we must take issue with the premise of the question, and say that the earth's"tilt" does in fact "stay the same".precession-apex answer
The change in Earth's tilt is called axial precession. This is the slow, cyclical wobble in Earth's axis that causes the tilt to change slightly over a period of approximately 26,000 years.
Earth's precession is believed to be one of the contributing factors to the ice ages, but it is not the sole cause. The most recent ice age, known as the Quaternary glaciation, began around 2.6 million years ago and ended approximately 11,700 years ago. This glacial-interglacial cycle was influenced by a combination of factors, including variations in Earth's orbit, tilt, and precession, as well as changes in atmospheric composition.
Earth's orbit influences climate primarily through variations in its shape (eccentricity), tilt (obliquity), and axial precession. These changes affect the distribution and intensity of sunlight received by different parts of the planet, leading to cycles of glacial and interglacial periods, known as Milankovitch cycles. For instance, increased tilt can enhance seasonal contrasts, while a more circular orbit can lead to milder climate variations. Together, these orbital changes significantly impact long-term climate patterns and trends.
the amount of sunlight an area receives creates its season #10.4
The tilt of Earth's axis changes in a process called precession over a very long period of time. I'd say it's long-term.