Astronomy Picture of the Day |
APOD: 1997 September 21 - Looking Down on Saturn
Explanation:
This picture of
Saturn could not have been taken from
Earth. No
Earth
based picture could possibly view the night side of Saturn
and the corresponding shadow cast across
Saturn's rings.
Since Earth is much closer to the
Sun than
Saturn, only the day
side of the planet is visible from the
Earth. In fact, this photo was taken
by the
Voyager 1 spacecraft as it flew by
Saturn
in November 1980. The
next spacecraft to approach Saturn will be
Cassini which is currently
scheduled to be launched later this year and reach Saturn in 2004.
APOD: 2000 January 29 - Natural Saturn On The Cassini Cruise
Explanation:
What could you see
approaching Saturn aboard
an interplanetary cruise ship?
Your view would likely resemble
this subtly shaded image of the gorgeous ringed gas giant.
Processed by the
Hubble Heritage project, the picture intentionally
avoids overemphasizing color contrasts and presents a
natural looking Saturn
with cloud bands, storms,
nearly edge-on rings, and the small round shadow
of the moon Enceladus near the center of the planet's disk.
Of course, seats were not available on
the only ship currently enroute - the Cassini spacecraft,
launched in 1997 and
scheduled to arrive at Saturn in the year 2004.
After an extended cruise to a world 1,400 million kilometers
from the Sun,
Cassini will tour
the Saturnian system,
conducting a remote, robotic exploration
with software and instruments
designed by
denizens of planet Earth.
But where is Cassini now?
Still about 980 million kilometers from Saturn, last
Sunday the spacecraft flew by
asteroid 2685 Masursky.
APOD: 1999 January 23 - Saturnian Aurora
Explanation:
Girdling
the second largest planet in the Solar System,
Saturn's Rings
are one of the most spectacular sights for earthbound
telescopes.
This image from the orbiting
Hubble Space Telescope's STIS instrument,
offers a striking view of another kind of
ring around Saturn -
pole encircling rings of
ultraviolet aurora.
Towering more than 1,000 miles above
the cloud tops, these Saturnian auroral
displays are
analogous to Earth's.
Energetic charged particles in
the Solar Wind are
funneled by the planet's magnetic
field into polar regions
where they interact with atmospheric gases.
Following the ebb and flow of Saturn's aurora, researchers can
remotely explore the planet's atmosphere and magnetic field.
In this false color image, the dramatic red aurora identify emission
from atomic hydrogen, while the more concentrated white areas are
due to hydrogen molecules.
In 2004, NASA plans to begin making close-up studies
of the Saturnian system with
the Cassini Spacecraft.
Authors & editors:
Robert
Nemiroff
(MTU)
& Jerry Bonnell (USRA)
NASA Technical Rep.:
Jay Norris.
Specific rights apply.
A service of:
LHEA at
NASA/
GSFC
&
Michigan Tech. U.