Notable Isotopes  |
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3He [1 neutrons] |
Abundance: 0.000137%
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Stable with 1 neutron
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Extraplanetary material, such as lunar and asteroid regolith, have trace amounts of helium-3 from being bombarded by solar
winds. The Moon's surface contains helium-3 at concentrations on the order of 0.01 ppm.[
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4He [2 neutrons] |
Abundance: 99.999863%
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Stable with 2 neutrons
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Liquid helium-4 can be cooled to about 1 kelvin using evaporative cooling. |
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5He [3 neutrons] |
Abundance:
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Half life: 7.00(30) x 10-24 seconds
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Decays to 4He.
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Highly unstable, decays to 4He.
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6He [4 neutrons] |
Abundance:
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Half life: 806.7(15) ms [ beta- ]
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Decays to 6Li.
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Produced from 7He or 11Li.
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7He [5 neutrons] |
Abundance:
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Half life: 2.9(5)-21 seconds
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Highly unstable, decays to 6He.
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8He [6 neutrons] |
Abundance:
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Half life: 119.0(15) ms
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Produced from 9He, decomposes to 7Li through beta decay then emits a delayed neutron.
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9He [7 neutrons] |
Abundance:
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Half life: 7(4) x 10-21 seconds
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Highly unstable, decays to 8He.
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10He [8 neutrons] |
Abundance:
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Half life: 2.7(18) x 10-21 seconds
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Highly unstable, decays to 9He.
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