Transcript Document

What do I already know?
I know what I can see in space using binoculars.
I know what a telescope is.
The suitability of optical
instruments
Produce an information leaflet or poster which
identifies at least THREE DIFFERENT methods (land
and space based) that scientists use to observe and
find out about the Universe. Describe the features
each has to make them suitable for their purpose.
Naked eye Binoculars Telescopes
What can you see in
space just using your
eyes?
Describe some of the
objects you can see.
What can you see in
space using
binoculars?
Describe some of the
objects you can see.
What can you see in
space using
telescopes AND
space based
telescopes?
Describe some of the
objects you can see.
Use pictures!!
Then:
Discuss on the suitability of each:
Which is the best to use? When? Why?
Think about poor weather conditions, daylight and electromagnetic waves.
Jupiter and its four largest moons roughly as
Lunar map showing the major features of the they will appear in a small telescope
Moon's surface
The Pleiades photographed using a 90 mm
(3.5 in) telescope
Orion's belt and sword. The bright fuzzy spot
on the sword is the Orion Nebula, a diffuse
nebula that appears about twice the size of
the full moon
Close-up view of the Trapezium asterism
within M42
The Large and Small Magellanic Clouds. Note
the enormous NGC104 globular cluster to the
left of the SMC
The Andromeda galaxy, M31, also showing
the satellite galaxies M32 and M110
M33, the Triangulum galaxy, clearly showing
the face-on spiral structure
Apollo 15 picture of Messier and Messier A
craters, clearly showing the long parallel
ejecta plumes
Jupiter as captured by the Cassini probe
http://chandra.harvard.edu/photo/2014/m106/
http://www.gizmag.com/top-five-astronomicalobjects-new-telescope/25600/pictures#21
https://www.astronomics.com/what-can-youexpect-to-see-in-a-telescope_t.aspx
The four largest moons of Jupiter, as imaged
by the Galileo spacecraft
http://hubblesite.org
Hubble's view of the Pleiades including star
names
Hubble mosaic image of the Great Orion
Nebula
Close-up of the Large Magellanic Cloud,
showing the reddish Tarantula Nebula above
the left end
Astrophoto of the Tarantula Nebula taken by a
robotic telescope with an aperture of 24 in
(0.6 m)
Close-up of the Small Magellanic Cloud. Note
the globular cluster NGC104 at the bottom of
the frame
Puppis A is a supernova remnant
located about 7,000 light years from
Earth.
This new image includes data from
Chandra and XMM-Newton and is the
most complete and detailed X-ray view
of Puppis A to date.
The combined dataset reveals a
delicate tapestry of X-ray light left
behind by the supernova explosion.
The core region of globular cluster NGC104
A new composite of NGC 4258 features X-rays from Chandra (blue),
radio waves from the VLA (purple), optical data from Hubble (yellow
and blue), and infrared with Spitzer (red).
NGC 4258 is well known to astronomers for having "anomalous" arms
that are not aligned with the plane of the galaxy, but rather intersect
with it.
Researchers are trying to understand how the giant black hole in the
center of NGC 4258 is affecting the rest of the galaxy.
NGC 4258, also known as Messier 106, is located about 23 million light
years from Earth.
The Hubble Space Telescope's launch in 1990 sped humanity to one of
its greatest advances in that journey. Hubble is a telescope that orbits
Earth. Its position above the atmosphere, which distorts and blocks
the light that reaches our planet, gives it a view of the universe that
typically far surpasses that of ground-based telescopes.
Hubble is one of NASA's most successful and long-lasting science
missions. It has beamed hundreds of thousands of images back to
Earth, shedding light on many of the great mysteries of astronomy. Its
gaze has helped determine the age of the universe, the identity of
quasars, and the existence of dark energy.
WHY A SPACE TELESCOPE?
The Hubble Space Telescope is the direct solution to a
problem that telescopes have faced since the very
earliest days of their invention: the atmosphere. The
quandary is twofold: Shifting air pockets in Earth's
atmosphere distort the view of telescopes on the
ground, no matter how large or scientifically advanced
those telescopes are. This "atmospheric distortion" is
the reason that the stars seem to twinkle when you look
up at the sky.
The atmosphere also partially blocks or absorbs certain
wavelengths of radiation, like ultraviolet, gamma- and Xrays, before they can reach Earth. Scientists can best
examine an object like a star by studying it in all the
types of wavelengths that it emits.
Newer ground-based telescopes are using technological
advances to try to correct atmospheric distortion, but
there's no way to see the wavelengths the atmosphere
prevents from even reaching the planet.
The most effective way to avoid the problems of the
atmosphere is to place your telescope beyond it. Or, in
Hubble's case, 353 miles (569 km) above the surface of
Earth.