1. the "s" process that occurs inside a star before it
unlike the "s" process that occurs process happens only during the of a star

2. when a star explodes into
a supernova, it produces a huge amount of
and releases an extremely high number of

3. these neutrons are then rapidly captured by the various nuclei that are rele
by the exploding star, producing new nuclei through the

with neutrons. pls fill in the blank. you

frequency, z, and the collision density, z, in carbon dioxide (co2), r 180 pm at 30 °c and 120 kpa

points

explanation:

percent abundance for cu-63 can be shown as:

63 x + 65 (1-x) = 62.9296

65 - 62.9296 = 2 x

x = 1.035

thus, percent abundance for cu-63 is 1.035

percent abundance for cu-65 can be shown as:

63 x + 65 (1-x) = 64.9278

65 - 64.9278 = 2 x

x = 0.0361

thus, percent abundance for cu-63 is 0.0361

the mass spectrum of cu-63 showing the intense peak as, this isotope is found in nature more abundantly around 92.38 % in comparison to cu-65 which is found 62.58 % naturally