Deep Space Objects

 

OBJECTIVES:

 

1.            Students will be able to locate nebulas, double stars, clusters, variable stars, and galaxies (in the StarLab).

2.            Students will be able to describe nebulas, double stars, clusters, variable stars, and galaxies.

3.            Students will be able to describe the location of “Mizar and Alcor” (a double star pair).

 

 

RELATION TO MISSOURI FRAMEWORKS:

 

9-12:  VA2            Stars appear to go through a cycle of birth, development, and death.

9-12:  VA3            Because of the vast distances between objects in the universe, light may take billions of years to reach Earth.

9-12:  VB1            Newton’s conception of the universe established the idea that the laws, which apply to processes that occur on the Earth, also apply to the universe.

9-12:  VC1            Space exploration has expanded our knowledge of the universe and advanced the technological sophistication of our society.

 

CONTEXT:

 

Grade Level:  8-12

            Group of 15-25 for StarLab presentation

 

PREREQUISITE:

 

The students should have an understanding of stars and constellations.

 

MATERIALS:

 

StarLab Portable Planetarium

            Starfield and Deep Space Objects Cylinders

Arrow pointers

Red Flashlight for reading text

 

PROCEDURE:

 

1.      When all students are seated, begin to ask questions to gauge their previous knowledge as their eyes get used to the darkness.  “What are stars?”  “What are constellations?”  “Can anyone name a constellation?”  “Can anyone find a constellation in the night sky?”

 


2.                  As the questions are asked and answered begin to turn up the StarLab lamp with the Starfield Cylinder in place.  “This is a simulation of the night sky if it is viewed away from the city.”  “What are we viewing?”  [Stars]  “Who can pick out any constellations here?”  (Pass the pointer to a volunteer.)

 

3.                  “Let’s change cylinders to get a different view of the night sky.”  Turn down the lights and change to the Deep Sky Objects Cylinder.  As you bring up the lamplight, “You just indicated that we were looking at stars in the night sky.  What do you see now?”

 

4.                  Indicate to the students that the symbols stand for different objects in the universe, many of which are outside of our galaxy, or are just too far away to be seen without binoculars or a telescope.  The star shapes represent nebulae, diamond shapes are variable stars, triangles are double stars, rectangular boxes are galaxies, and square shaped objects represent clusters. [Point out the location of one or two during the explanation of symbols.

 

5.                  Explain what each of the objects is and how studying it has helped in furthering  understanding in the field of Astronomy.

 

Nebulae:   An accumulation of gas and dust.  Usually about 90% Hydrogen, 8% Helium and 2% other elements. Studying Nebulae have increased astronomers understanding of the life cycle of stars.  These are the birthplace of stars.  Gravity pulls the gasses together until the added pressure causes fusion.  Nebulae can also be related to the death of stars.  As stars lose mass, its gravitational pull is reduced and gases are lost to the surrounding space.

 

Double Stars: Even though we normally see one point of light with our eyes, more than half of the stars in the Milky Way Galaxy are actually twins.  That makes our sun part of a galactic minority.  These double stars appear to revolve around each other, but in reality orbit a common center of mass between them.

One of the best known and easiest to find pairs are “Mizar” and “Alcor.”  These two stars make up the “second star” in the handle of the Big Dipper.

 

Variable Stars:  Though most stars give off a relatively constant amount of energy (light), some appear to change brightness on a regular basis.  Some change brightness because of mutual eclipses of double stars.  Others are stars, which actually change in size and temperature.  These stars are thought to be near the end of their life cycle and vary in brightness because their fuel is nearly exhausted.

 


Clusters: Because they form from nebulae, stars seldom form alone.  Instead, they form in groups, associations, and clusters.  Gravity is the deciding factor for all clusters.  If the gravitational force is weak, the stars drift apart forming an open cluster. [The Big Dipper of Ursa Major is an association of stars (open cluster) that is drifting apart.] There are two types of clusters, open clusters that are thought to be relatively young on the cosmic time scale, and globular clusters, which are thought to be the oldest stars in the galaxy.

 

Galaxies: All the stars, clusters, and nebulae seen with the unaided eye are part of the Milky Way Galaxy.  The Milky Way is just one of millions or perhaps billions of galaxies in the universe.  The locations of many of these galaxies have been known for decades.  When we leave, you will receive a handout that will show the locations of many galaxies that are visible with binoculars.

 

6.                  “Why can’t the Andromeda Galaxy or other Deep Sky Objects be viewed with the naked eye?” [Because of their great distances, they are too dim to be seen.]

 

7.                  “Who can point out and describe a nebula; double star; variable star; cluster; galaxy?”

 

8.                    Let’s go outside where you will have a short evaluation and get your “Sky Map” so you can look for some of these objects at home. [Bring up the side lamps and turn down the projection lamp so students may exit the StarLab.]

 

 

REFERENCE:

 

1.            The Talcott Mountain Science Center, “A Look at the Deep Sky Cylinder,” Astronomy and More: Activities for the StarLab Portable Planetarium.

 

2.                  Kratzer, Gary D., “Deep Sky Objects: Activity 1,” Astronomy and More: Activities for the StarLab Portable Planetarium.

 

3.                  Anonymous, “Celestial Objects: Northern Hemisphere, July, 2000,” 2 pages.  Available: http:www.skymaps.com/store [July 27, 2000]

 

 

 

EXTENSIONS AND/OR ADAPTATIONS:

 

Upon completion of the evaluation sheet, pass a list of Deep Sky Objects and Sky Maps to the students.  Ask them to try to find any of the objects listed in the sky this evening.  (Remember, most require binoculars or a telescope.)

 

CONTENT BACKGROUND:

 


Because of the vast distances between objects in the universe, our view of the night sky is limited by sensitivity of our sensors.  When viewing the sky with our eyes, we are limited in our ability to gather and focus light.  Because of these limitations, humans can only see the celestial objects, which appear bright.  These objects usually appear bright because they are close.  Every star like object we can see with the unaided eye is in our own Milky Way Galaxy.  There is a vast universe beyond The Milky Way, as well as faint objects within the Milky Way that are normally too dim to see without magnification.  Objects such as Nebulae, Double Stars, Clusters, Variable Stars and other Galaxies.

 

APPENDIX:

 

1.                  Post activity evaluation sheet.

2.                  Sky Map for the month with the celestial objects listed.

 

WEB SITES:

 

www.britannica.com/bcom/eb/article - (online encyclopedia)

www.sciam.com/1998/1098issue/1098laham.html - (online periodical)

www.cobweb.nl/bertyvon/index.html - (Images and descriptions of Deep Sky Objects)

www.skymaps.com/store (Monthly maps of the night sky with glossary)

 

 


  Deep Sky Objects

 

 Provide an accurate description for each of  the following Deep Sky Objects.  As a bonus, how has the study of any of the those objects increased mankind’s knowledge of  star life cycles and/or star masses.

 

Nebulae

 

 

 

 

 

 

Double Stars

 

 

 

 

 

 

Clusters

 

 

 

 

 

 

Variable Stars

 

 

 

 

 

 

Galaxies

 

 

 

 

 

 

What are “Mizar” and “Alcor” and where can they be found in the night sky?