Tuesday, April 24, 2012

AMAZING! Northern Lights from ISS

Friday, April 13, 2012

MOONKAM

Happy Vacationing Students,

Our first images of the moon are coming back.  If you need more codes let me know at jsneideman@tarbut.com
IMAGE_52673
Photo ID52673
Schooltarbutv1
Time Taken (UTC)2012/096/11:38:13
Orbit1274
SpacecraftEbb
Camera DirectionBackward
Lens (mm)6.00
Altitude (km)48
Frame Width (km)0.00
Frame Height (km)48.23
Nadir61.54° S, 61.71° W
Center58.5° S, 62.89° W
IMAGE_8095

IMAGE_8108

IMAGE_52673


IMAGE_52678IMAGE_52674
h
ttp://images.moonkam.ucsd.edu/v/MK12_03/1177_0T840TA600000_37886_2012-088-21_13_42_000_2012-088-21_13_58_508.bmp.html

Thursday, March 8, 2012

Rubric for Rover Project

Awards for
  • Fastest Acceleration (3 trials average)
  • Furthest Distance Traveled (3 trials average)
  • Top Average Speed (3 trials average)
  • Vote for Best Design
8th grade NASA ROVER DESIGN CHALLENGE RUBRIC
PHASE  I.  DESIGN PHASE
Pts
CRITERIA

Mission statements
20
·         Statement of purpose
·         Goals of mission are clear and accurate
·         List and explanation of scientific instruments to be used


Work log /Blog**
20
You keep track of your daily accomplishments, learning, and individual work done – signed off by team leader and/or teacher
(photo log on team blog is evidence of work done)

Design of rover
30
·         List of materials included
·         3 views of your design (top, side, oblique)
·         Labeled parts
·         Design includes logo
·         Includes scientific instruments
·         TO SCALE**

Slogan/Logo
20
·         Creative, appropriate, relevant, colorful and DIGITAL –
·         Emailed to Mr. S          jsneideman@tarbut.com
·         Included on your blog
·         Theme song **


Kindergarten Project 1
20
·         You have something prepared for your kindergarten team members to work on when you present the topic.  (coloring which will be included on the final project)

PHASE II. BUILDING PHASE
Building (daily grade)
20
Points will be taken off of the entire team members are idle.  Needs to be evidence of progress daily.

Finished design resembles design
20
The percent similarity of your prebuilding design and your finished project.

Finished project
50
·         Solidly built – not falling apart
·         creativity
·         Moves down a hill by the force of gravity and or with a push
·        

Presentation to the board
50
·         3-5 minute presentation
·         Clearly demonstrates knowledge about

Kindergarten Project 2
20
TBA

PHASE III. EXPERIMENTING PHASE
Newton’s Law Lab
50
TBA

Lab Report
50
Complete lab report : Includes all sections from lab rubric

Finished **Blog of Progress
50
TBD

Kindergarten Project 3
20
Presentation

Other



Tuesday, February 14, 2012

Study Guide Chapter 19


Study Guide Test on Chapter 19.
Understand the phases of the moon.
Understand the H-R diagram
Understand the temp/color/composition of stars
Understand the difference between galaxy types
Understand the big dipper is like a clock and how to read that clock.
Know how to use a star tracker.
Explain the life cycle of a star depending on its starting mass.
Know galaxy worksheet - basics of galaxies and black holes and super galaxies
Understand the meaning of each variable in the Drake equation.  F sub capital L?

Essay: Explain the cuases of the seasons in detail.  Give examples using the Poles and Tropic Lines.

Spectrum
Apparent magnitude
Absolute magnitude
Light-year
Parallax
H-R diagram
Main sequence
White dwarf
Red giant
Supernova
Neutron star
Pulsar
Black hole
Galaxy
Spiral galaxy
Elliptical galaxy
Irregular galaxy
Nebula
Open cluster
Globular cluster
Quasar
Gibbous
Crescent
Waxing
Waning
Solstice
Equinox
Aphelion
Perihelion
Angular Heigth of the Sun


Honors:
·         Math using speed of light and scientific notatio
·         Math calculating the distance and time to travel to certain stars or size and distance between galaxies calculated.
·         Use the Drake equation given certain variables
·        What is Dark Matter and Dark Energy?



Do Now: Stars Spectra

What does the surface color of a star tell us? Explain in detail. Then explain what is an absorption spectra.





Sources of continuous, emission, and absorption spectra




Sources of continuous, emission, and absorption spectra



http://csep10.phys.utk.edu/astr162/lect/light/absorption.html
Thus, emission spectra are produced by thin gases in which the atoms do not experience many collisions (because of the low density). The emission lines correspond to photons of discrete energies that are emitted when excited atomic states in the gas make transitions back to lower-lying levels.

A continuum spectrum results when the gas pressures are higher. Generally, solids, liquids, or dense gases emit light at all wavelengths when heated.

An absorption spectrum occurs when light passes through a cold, dilute gas and atoms in the gas absorb at characteristic frequencies; since the re-emitted light is unlikely to be emitted in the same direction as the absorbed photon, this gives rise to dark lines (absence of light) in the spectrum.