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formati

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The answer FORMATI has 0 possible clue(s) in existing crosswords.

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The word FORMATI is NOT valid in any word game. (Sorry, you cannot play FORMATI in Scrabble, Words With Friends etc)

There are 7 letters in FORMATI ( A¹F⁴I¹M³O¹R¹T¹ )

To search all scrabble anagrams of FORMATI, to go: FORMATI?

Rearrange the letters in FORMATI and see some winning combinations

6 letters out of FORMATI

FORMAT MAFTIR

5 letters out of FORMATI

AFRIT AMORT FORAM MOIRA MOTIF RATIO

4 letters out of FORMATI

3 letters out of FORMATI

AFT AIM AIR AIT AMI ARF ARM ART FAR FAT FIR FIT FOR FRO MAR MAT MIR MOA MOR MOT OAF OAR OAT OFT ORA ORT RAI RAM RAT RIA RIF RIM ROM ROT TAM TAO TAR TOM TOR

2 letters out of FORMATI

AI AM AR AT FA IF IT MA MI MO OF OI OM OR TA TI TO

Searching in Dictionaries ...

Definitions of formati in various dictionaries:

FORMATI - The formation and evolution of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular clou...

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Formati might refer to
The formation and evolution of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed. * This model, known as the nebular hypothesis and now refined as the Nice model (2005), was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990's, the model has been both challenged and refined to account for new observations. * The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as Earth's Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution. * In roughly 5 billion years, the Sun will cool and expand outward to many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.

Formati might refer to

The formation and evolution of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.
* This model, known as the nebular hypothesis and now refined as the Nice model (2005), was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990's, the model has been both challenged and refined to account for new observations.
* The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as Earth's Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.
* In roughly 5 billion years, the Sun will cool and expand outward to many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.

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