Across
- 2. The primordial, simplest, and most abundant element, created within the first 3 to 20 minutes of the universe’s existence through nucleosynthesis, forming roughly 75% of ordinary matter by mass.
- 4. The scientific study of the origin, evolution, and structure of the universe.
- 5. American astronomer who provided the foundational observational evidence for the Big Bang theory by proving the universe is expanding.
- 10. An American astronomer who, along with Arno Penzias, accidentally discovered the Cosmic Microwave Background radiation in 1964.
- 13. The faint, nearly uniform, remnant heat left over from the Big Bang, filling all space in the observable universe.
- 16. Massive, gravitationally bound systems formed from the coalescence of primordial gas and dark matter as the early universe cooled.
- 17. The second-lightest and second-most abundant element, forming about 24%–25% of the total mass of the universe.
- 18. The pinnacle of scientific genius, specifically for his work on relativity.
Down
- 1. A German-American physicist who, with Robert Wilson, serendipitously discovered the Cosmic Microwave Background radiation in 1965.
- 3. British astronomer who famously coined the term "Big Bang" during a 1949 BBC radio broadcast to describe a theory he strongly opposed.
- 6. The entire range of radiation emitted by the early universe, which has since been stretched by expansion into the cosmic microwave background.
- 7. All of space,time,matter, and energy.
- 8. The narrow range of electromagnetic radiation that the human eye can detect, spanning from violet to red.
- 9. The prevailing scientific model explaining that the universe began approximately 13.8 billion years ago from an extremely hot, dense point and has been expanding and cooling ever since.
- 11. An instrument that splits light from astronomical objects into a spectrum, used to determine composition, temperature, and velocity.
- 12. The foundational substance of the universe, representing the high-density, rapidly expanding primordial state that converted into all matter and radiation.
- 14. The increase in wavelength (stretching) of light from distant galaxies as it travels through expanding space.
- 15. The compression of light waves from an object moving toward an observer, shifting its light toward the blue-violet end of the spectrum.
