›› Convert megalight year to gigalight year


megalight-year
gigalight-year


›› More information from the unit converter

How many megalight-year in 1 gigalight-year? The answer is 1000.
We assume you are converting between megalight year and gigalight year.
You can view more details on each measurement unit:
megalight-year or gigalight-year
The SI base unit for length is the metre.
1 metre is equal to 1.0577248071986E-22 megalight-year, or 1.0577248071986E-25 gigalight-year.
Note that rounding errors may occur, so always check the results.
Use this page to learn how to convert between megalight years and gigalight years.
Type in your own numbers in the form to convert the units!


›› Quick conversion chart of megalight-year to gigalight-year

1 megalight-year to gigalight-year = 0.001 gigalight-year

10 megalight-year to gigalight-year = 0.01 gigalight-year

50 megalight-year to gigalight-year = 0.05 gigalight-year

100 megalight-year to gigalight-year = 0.1 gigalight-year

200 megalight-year to gigalight-year = 0.2 gigalight-year

500 megalight-year to gigalight-year = 0.5 gigalight-year

1000 megalight-year to gigalight-year = 1 gigalight-year



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›› Common length conversions

megalight-year to pike
megalight-year to petameter
megalight-year to canna
megalight-year to fist
megalight-year to X unit
megalight-year to pica
megalight-year to pace
megalight-year to kilometer
megalight-year to chinese yard
megalight-year to zettameter


›› Definition: Megalight-year

One megalight-year, abbreviated "Mly", is one million light-years, or 306,601 parsecs. Megalight-years are typically used to measure distances between neighboring galaxies and galaxy clusters.


›› Definition: Gigalight-year

One gigalight-year, abbreviation "Gly", is one billion light-years — one of the largest distance measures used. One gigalight-year equals 306.601 million parsecs, or roughly one-thirteenth the distance to the horizon of the observable universe (dictated by the cosmic background radiation). Gigalight-years are typically used to measure distances to supergalactic structures, such as clusters of quasars or the Great Wall.


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