Crossword Solver > found answer > VABLES

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vables

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

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

There are 6 letters in VABLES ( A1B3E1L1S1V4 )

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

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Scrabble results that can be created with an extra letter added to VABLES

ABSOLVE VERBALS SAVABLE

5 letters out of VABLES

ABLES BALES BLASE LAVES SABLE SALVE SELVA SLAVE VALES VALSE VEALS

4 letters out of VABLES

ABLE ALBS ALES AVES BALE BALS BASE BELS BLAE LABS LASE LAVE LAVS LEAS LEVA SABE SALE SAVE SEAL SLAB VALE VASE VEAL VELA

3 letters out of VABLES

ABS ALB ALE ALS AVE BAL BAS BEL BES ELS LAB LAS LAV LEA LES LEV SAB SAE SAL SEA SEL VAS

2 letters out of VABLES

AB AE AL AS BA BE EL ES LA

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Definitions of vables in various dictionaries:

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Vables might refer to
Valles Marineris (Latin for Mariner Valleys, named after the Mariner 9 Mars orbiter of 1971–72 which discovered it) is a system of canyons that runs along the Martian surface east of the Tharsis region. At more than 4,000 km (2,500 mi) long, 200 km (120 mi) wide and up to 7 km (23,000 ft) deep, Valles Marineris is one of the largest canyons of the Solar System, surpassed in length only by the rift valleys of Earth.
* Valles Marineris is located along the equator of Mars, on the east side of the Tharsis Bulge, and stretches for nearly a quarter of the planet’s circumference. The canyon system starts in the west with Noctis Labyrinthus; proceeding to the east are Tithonium and Ius chasmata, then Melas, Candor and Ophir chasmata, then Coprates Chasma, then Ganges, Capri and Eos chasmata; finally it empties into an outflow channel region containing chaotic terrain that ends in the basin of Chryse Planitia.
* It has been recently suggested that Valles Marineris is a large tectonic "crack" in the Martian crust. Most researchers agree that this formed as the crust thickened in the Tharsis region to the west, and was subsequently widened by erosion. Near the eastern flanks of the rift, there appear to be channels that may have been formed by water or carbon dioxide. It has also been proposed that Valles Marineris is a large channel formed by the erosion of lava flowing from the flank of Pavonis Mons.
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