Astronomy Notes – Unit 1 – Sun

 

WARNING:  Never, ever look directly at the Sun, especially with binoculars or telescopes!

 

q       (1) The Sun is the nearest star to Earth, at an average distance of _________ miles (150 million kilometers).  Since the speed of light is _______________________, it takes about _______________ for light from the Sun to reach the Earth.

q      (2) The diameter of the Sun is 875,000 miles (1.4 million kilometers). It could hold more than __________ Earths.

q      (3) The surface gravity of the Sun is about ____ times that of the Earth.

q      (4) The Sun produces huge amounts of energy, including light and heat, from a process called nuclear fusion. This process joins pairs of ____________ atoms into ___________ atoms.

q       (5) Scientists believe the temperature of the Sun varies from ___________ degrees Fahrenheit (15 million degrees Celsius) at the core, to ________ degrees Fahrenheit (5,500 degrees Celsius) at the surface, or photosphere.

q      (6) The corona (Latin for crown) is the outer part of the Sun’s atmosphere, and is visible during a ______________.

q      (7) The Sun’s average period of rotation about its axis varies from ­­­­­­________ at the equator to __________ at higher latitudes.

q      (8) A sunspot is a temporary, darker, cooler patch on the surface of the Sun. These are believed to be caused by magnetic fields that impede hot gases from rising to the surface.  They last about a week or so. A typical sunspot is about the
_____________ or larger.

q      (9) Massive, violent explosions of hot _________ on the Sun’s surface are called solar flares. These can last from a few minutes to a few hours.

q      (10) The Sun continually emits a stream of high energy, electrically charged particles called the solar wind. Near Earth, the average speed of the solar wind is about ___________________ (450 million kilometers/hour).

q      (11) The limit of the solar wind extends beyond the orbit of Neptune.  The _______ spacecraft are searching for the heliopause, the boundary where the solar wind no longer exists.

q      (12) The Earth’s magnetic field protects us from the solar wind.  These particles cause colorful, rippling lights called aurora borealis, or _______________ near the north pole, and aurora australis, or ______________ near the south pole.

q      (13) Surges in the solar wind caused by solar flares can disrupt communications and power transmission here on Earth.

q      (14) Ultraviolet radiation from the Sun causes suntan and sunburn, and may be a factor in causing ______________.

 


Vocabulary

 

1)     Solar Wind:  ______________________________________________________
__________________________________________________________________

2)     Solar Flare:  ______________________________________________________
__________________________________________________________________

3)     Sunspot:  _________________________________________________________
__________________________________________________________________

4)     Photosphere:  _____________________________________________________
__________________________________________________________________

5)     Corona:  _________________________________________________________
__________________________________________________________________

6)     Astronomical Unit (A.U.):  __________________________________________
__________________________________________________________________

7)     Solar Prominence:  _________________________________________________
__________________________________________________________________

8)     Nuclear Fusion:  ___________________________________________________
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9)     Aurora Borealis (Northern Lights):  __________________________________
__________________________________________________________________

10) Aurora Australis (Southern Lights):  __________________________________
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