chapter 16 chat gpt notes

0.0(0)
Studied by 0 people
call kaiCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/25

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 8:15 PM on 6/14/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai

No analytics yet

Send a link to your students to track their progress

26 Terms

1
New cards

Sun radius

700,000 km

2
New cards

Photosphere temperature

5800 K

3
New cards

Core temperature

15 million K

4
New cards

Luminosity of the Sun

4 × 10²⁶ W

5
New cards

Solar constant

1400 W/m²

6
New cards

Equatorial rotation period of the Sun

25 days

7
New cards

Sunspot cycle duration

11 years

8
New cards

Full magnetic cycle duration

22 years

9
New cards

Corona temperature

Approximately 3 million K

10
New cards

Solar wind speed

Approximately 500 km/s (up to 800 km/s from coronal holes)

11
New cards

Core

The center of the Sun where nuclear fusion occurs converting hydrogen to helium.

12
New cards

Proton-Proton chain

The primary fusion process in the Sun that combines four hydrogen nuclei into one helium nucleus.

13
New cards

E=mc²

Equation describing the mass-energy equivalence used in nuclear fusion.

14
New cards

Helioseismology

The study of solar vibrations used to learn about the Sun's interior.

15
New cards

Granules

Small, bright features on the Sun's surface caused by convection, about 1000 km across.

16
New cards

Spicules

Jets of gas in the chromosphere, approximately 100 km/s, lasting a few minutes.

17
New cards

Coronal holes

Regions of lower density in the corona where solar wind primarily escapes.

18
New cards

Sunspots

Dark spots on the photosphere caused by cooler temperatures due to strong magnetic fields.

19
New cards

Maunder Minimum

Period from 1645–1715 with almost no observed sunspots, associated with colder climate.

20
New cards

Solar flares

Explosions on the Sun that can produce X-rays and UV radiation.

21
New cards

Coronal Mass Ejection (CME)

A huge bubble of magnetized gas ejected into space capable of affecting Earth.

22
New cards

Neutrinos

Tiny particles produced during fusion with almost no interaction with matter.

23
New cards

Neutrino oscillation

The phenomenon of neutrinos changing type while traveling, discovered during the solar neutrino problem.

24
New cards

Granulation

The pattern of bright centers (hot gas rising) and dark edges (cool gas sinking) seen on the Sun's surface.

25
New cards

Differential rotation

The Sun's rotation varies with latitude; equator rotates faster than poles.

26
New cards

Solar activity impact on Earth

Can cause auroras, satellite disruptions, GPS issues, radio communication problems, and power outages.