Celestial
Bodies (Stars & Constellations)
Reflection
VS Sources of Light
The
students will review some facts about light learned in Grade 2, specifically
that some objects emit light; some objects reflect light, and some objects
absorb light and that light is a radian wave emitted from a source in straight
lines and spreads over a larger and larger area as it travels. Students will be able to demonstrate why,
although the stars are always shining, they are ordinarily visible only at
night. Students will be able to explain
why some objects like the Sun, and sometimes the Moon, are visible during the
day.
Comets,
Meteors, and Meteorites
Specifically,
students will explain that a comet is a large ball of frozen gases, dust, and
ice that glows brightly as it approaches the Sun, that it travels in a long,
cigar-shape orbit around the sun, and that the comet’s tail always points away
from the Sun because strong solar wind coming from the Sun blows the glowing
gases backward off the comet. Students
will be able to define meteors as bits of rock or dust, often from the tail of
a comet, that burn up as they fall through the earth’s atmosphere. Students will be able to define a meteorite
as a chunk of rock that does not completely burn up as it travels through the
earth’s atmosphere and that when a meteorite hits land it causes a resulting
crater.
·
Comets
The Life
Cycles of Stars
The
students will be able to characterize stars by size and color: red giant, white
dwarf, black dwarf, and black hole, and will be able to identify how these
characteristics relate to stages in the “life” cycle of a star. Students will be able to explain that stars
do not stay the same forever, stars are “born”, go through generally
predictable stages, and finally “die”, and that these stages represent the
“life” cycle of a star. Students will be
introduced to a possible, although uncommon, end to a star’s “life” cycle as a
nova or supernova.
1.
Nebula:
Butterfly
Nebula; Corina
Nebula; Orion
Nebula
2.
Protostar:
Chandra
Protostar; Protostar
3.
Star:
Sun;
4.
Red
Giant: Chandra
Red Giant;
5.
White
Dwarf: Chandra
White Dwarf; Sirius
White Dwarf; White
Dwarf Illustration
6.
Black
Dead Star: Black
Dwarf Solar Ashes; Cinders
in Space
7.
Nova:
Nova;
8.
Supernova:
Supernova
Remnent; Supernova
Crab Nebula
Our Sun
The
students will be able to identify stars, including our Sun, as providers of
heat and light. Students will be able to
demonstrate that when the Sun’s rays strike a surface, some are absorbed while
others are reflected, that the absorbed rays make things hotter, and the
reflected rays make things brighter.
Students will be able to identify sunlight a slight by showing that it
is made up of the same spectrum of colors as light produced by a
flashlight.
Constellations
The
students will be able to define constellations as groups of stars that are
named for what they look like. Students
will be able to demonstrate that the reason stars appear to move across the
night sky is not because they themselves are moving (although they are), but
because Earth is rotating and revolving.
Students will be introduced to the ways in which stars can be used to
find directions and tell time.
·
Constellations &
Their Stars
General Space
Sources
Back
to the Grade 3 With Mrs. Nelson Home Page