Write the nuclear equation for the fusion of two H-2 atoms to form He-3 and one neutron.
Step 1 of 3
Stellar Evolution Low Mass Stars Zero Age Main Sequence o Fusion begins o Main sequence life begins o Initial Mass determines future luminosity and temperature Stellar Sizes Red Dwarf o 1/25 – 1/10 M sun Low Mass o ¼ - 4 M sun Intermediate Mass o 4 – 25 M sun High Mass o 25 – 100+ M sun Not Now, Not Ever Brown Dwarf o Not a star – mass is too low for fusion ~50 Jupiter masses Low mass = Low pressure = Low core temp o Will “shine” in infrared Heat released from friction and cooling Does not generate its own energy Red Dwarf 0.08 M sun o M-type
Textbook: Introductory Chemistry
Author: Nivaldo J Tro
This textbook survival guide was created for the textbook: Introductory Chemistry, edition: 5. Since the solution to 85P from 17 chapter was answered, more than 385 students have viewed the full step-by-step answer. Introductory Chemistry was written by and is associated to the ISBN: 9780321910295. The full step-by-step solution to problem: 85P from chapter: 17 was answered by , our top Chemistry solution expert on 05/06/17, 06:45PM. The answer to “Write the nuclear equation for the fusion of two H-2 atoms to form He-3 and one neutron.” is broken down into a number of easy to follow steps, and 17 words. This full solution covers the following key subjects: atoms, equation, form, fusion, neutron. This expansive textbook survival guide covers 19 chapters, and 2046 solutions.