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Astronomy Club of Augusta
2017-2018

SEED Information
October 07, 2017, Saturday, 10AM - 3PM
set up & registration, 8:00-10AM

If you came to this webpage and would like to volunteer,

but are not listed below, please email.

Volunteers

 

Fri. 10AM Load the truck: Stan, Tedda,
Sat. 8:00AM  Set up at RPSEC: Help from ALL members.
Thanks to Baker White for loan of one T-Post Pounder.


Tedda Howard S       DH Solarscope                                                 <10am -3pm>

Gloria Sloan      S

Tedda Howard  M       Sun size, distance, temperature, brightness       T-shirt & Lunch distribution:

Helen Miller         M

Kenneth Beard   L       Solar Structure

Vinay Kolar       L       Solar Scope   

SusanBlas          L       Sun: Computer Power Point Loop                                                     

John Blas           L

Stephen Miller   L        Solar Scope

Mike Close         L       Solar Cycles

Bruno Huguet    L        Solar Scope

Stan Howard    XL       Televue w Solar Filter                         8:30-9:30AM Pics/Video StanH

Aishu Kolar      XL      

John White      XL        Indirect Solar Projection box, shoe box projectors

Cassel Sloan  XL        Electromagnetic Spectrum 

                                   

Indoors:

Mark Moffatt   3XL          Station 2a. 10:00-12:30      Zooniverse

Adela Dziekanowski  3XL    Station 2b. 12:30- 3:00       2018 Parker Solar Probe 

 

2:45PM Everyone:. Load/Clean up.  Thank you!



We need MORE volunteers!
strong arms,

string tie-ers,
 Welcome and Registration

Darth Vader Bucket Head Viewers

Direct solar views with Welder Glass

Indirect DarthVader solar views, shoe box projectors, cards,

Solar spacecraft: at LaGrange points, encircling Sun,

Sun-Earth relationships:  CMEs, Van Allen Belts, . . .

Sticker/bookmark/photo hand outs

Bubbles  

Please email.


Thank you for volunteering for SEED again this year. It is a great experience.
We can assure first timers that at the end you will feel tired, but rewarded!

Please bring your sun, solarscope, spectroscope, solar viewers, and other solar projects.

If you have posters or information that we can put on our Solar Astronomy bulletin board,
please let us know, and bring it/them with you, or to our meetings beforehand.

Thanks for being involved!

Stan Howard
VP Observing


Here are some suggestions to help everyone:
Take care of yourself with HAT, sun block, long sleeve shirt, pants or long skirt,
Bring your equipment, project, etc. - anything about the sun! and/or The DAWN Mission
Come early: We will be here at 8:00AM to
set up equipment, pass out free t-shirts and ID tags, set up posters, get organized.
You will also get a Free Lunch.
Please come and help.

Thank you.




Trivia Question 2017:  What temperature is the visible surface of the sun?  the corona?

 

Answer:   Photosphere is 5800 K,  Corona is 1-3 million K.  

 

No wonder the sun's rays seem bright and still feel hot when they reach Earth!

 

Temperature Conversion table in  K=Kelvin, C=Centigrade, F= Farenheit

  1-3 million     K                                                Corona

          5800     K                                                 Photosphere

            373     K     100      C      212       F        boiling point of water at sea level

            310.15K       37      C        98.6    F        human body temperature

            273     K         0      C        32       F        freezing point of water into ice at sea level 

                0     K    -273.15 C     -459.67  F       absolute zero

 

The sun's corona is much hotter (by a factor from 150 to 450) than the visible surface of the Sun.  The photosphere's average temperature is 5800 kelvins compared to the corona's one to three million kelvins.

The corona is 10−12 times as dense as the photosphere, and so produces about one-millionth as much visible light.

 

https://www.bing.com/search?q=temperature+of+sun+surface%2C+corona%3F&form=EDGHPT&qs=PF&cvid=406e60b550234d8ab3618ce032875b8b&cc=US&setlang=en-US

https://en.wikipedia.org/wiki/Corona

https://www.thoughtco.com/chemistry-temperature-conversion-table-4012466

http://www.answers.com/Q/What_is_the_average_body_temperature_degrees_kelvin_and_celsiuses?#slide=2

http://www.csgnetwork.com/tempconv.html

 

 

                                              Trivia Questions  2016:               

A. What are the 4 requirements for a DWARF PLANET?
B. Name the 5 dwarf planets accepted by the IAU, in order.
C. Where are we searching for more?

                                               Answer:

                                           A. The IAU defines a "dwarf planet" as a celestial body that
1. is in orbit around the Sun,
2. has sufficient mass for its gravity to form a nearly round shape,
3. has NOT cleared the neighborhood around its orbit, and
4. is not a satellite.

All other objects orbiting the Sun, except planets and satellites,
shall be referred to collectively as "Small Solar System Bodies."

                                           B. The IAU has declared 5 to be dwarf planets: Ceres, Pluto, Haumea, Makemake, Eris (the largest).
                                                          Brown currently identifies eleven known objects—the five accepted by the IAU plus
                                                          2007 OR10, Quaoar, Sedna, Orcus, (307261) 2002 MS4 and Salacia—as "virtually certain",
                                                          with another dozen highly likely, and possibly >10,000 beyond the Kuiper Belt.

                                            C. The Kuiper Belt and the Oort Cloud.


                                           Trivia Question 2015:
What are three propulsion sources used in outer space by the
DAWN Mission spacecraft or the New Horizons spacecraft?

                                            Answer: 1. Gravity Assist (Slingshot), 2. Ion Propulsion, 3. Hydrazine(chemical rocket).
Ion propulsion makes efficient use of the onboard fuel
by accelerating it to a velocity ten times that of chemical rockets.
This efficiency is measured in terms of the specific impulse of the fuel (Isp).
- See more at:  
http://dawn.jpl.nasa.gov/mission/ion_prop.asp#sthash.3QCszH9X.dpuf
Ion thrusters create very low levels of thrust compared to conventional chemical rockets
but achieve very high specific impulse, or propellant mass efficiencies,
by accelerating their exhausts to very high speed.



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