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Starry Skies Above Santa Monica
June 26 - July 3, 2002
Mirek Plavec
Emeritus Professor of Astronomy,
UCLA
The Sun
- Slowly Returning to the South
Really very, very slowly. The turn-over time was the
summer solstice early on Friday, June 21, but the change will be hard
to notice for some time. Thus, on Sunday, the last day of June, the
Sun will rise at 5:45 (three minutes later than a week ago), and set
by 8:08 p.m. – actually just one minute later (!) than a week ago.
This rather surprising later sunset is due to the fact that the Sun
will culminate at 12:57 p.m., while a week ago this happened at 12:55.
As you can see, we can easily forget these insignificant details. You
may think that astronomers should have more important problems to deal
with, and they really do – all of the above is our heritage from a
distant past, yet still valid.
The Summer Moon
The Full Moon occurred on June 24, and this coming week, the Moon
will gradually lose part of its bright face, and recede into the
night. I must say that it will recede rather reluctantly. The reason
is that the Full Moon occurs very low, between Scorpius and
Sagittarius, practically at the place where the Sun is at its lowest
just before Christmas. And after that, the Moon will be moving ever
higher along the ecliptic, just what the Sun does after the New Year.
Since the Moon moves much faster than the Sun, the intervals between
its successive rising will be quite short – for example: on June 26,
it will rise by 10:07 p.m., and the next evening, it will rise only 41
minutes later, at 10:48.
During the entire week between the two Wednesdays, the Moon will
travel from Capricorn through Aquarius into Pisces, and will
eventually rise after midnight. Its Last Quarter will come on July 2.
Venus, the Lone Planet of our Evenings
A few days ago, I was still able to spot Jupiter fairly low above
the western horizon, but the domination of this celestial king is
coming to its end. Jupiter is now setting less than one hour after
sunset, and will be quickly lost in the glare above the western
horizon.
The only remaining evening planet is, however, the most beautiful
one, Venus. It is projected between the constellations Cancer (the
Crab) and Leo (the Lion), and is gradually approaching the brightest
star of Leo, Regulus. The two will be fairly close together on July
10. At present, Venus sets by 10:30 p.m., and is so bright that it
cannot escape your attention if you look to the west already some 40
minutes after sunset.
Perhaps it would be fair to Mercury to mention that it is currently
rising by 4:30 a.m., that is, more than one hour before the Sun, and
is fairly bright, but I can hardly expect that anyone in Santa Monica
to rise that early to see Mercury above the glare of all the city
lights to the east of you… There will be better times to look for this
fast-moving planet!
The Stars of our Summer Evenings
The Moon will slowly recede into the night, and if city lights
permit, you may be able to see the brightest stars of our summer sky.
After all, the end of the school year means the beginning of summer
vacations at places much more favorable for star watching!
It is not difficult to find and identify the brightest stars! The
search can best start with Venus, which is so bright that you cannot
miss it. As I mentioned above, Venus will pass close to Regulus in Leo
on July 10, so the two objects will be close to each other for several
nights about this date. Venus will then continue along the ecliptic to
the south-east, but your eyes can move much faster than the planet. It
will be fairly easy to find the next bright star along the ecliptic,
Spica, in the constellation of Virgo.
The next constellation along the ecliptic is Libra (the Scales),
but it has no bright stars. You have to continue further to the
southeast to find the next first-magnitude star, Antares in Scorpius,
which has a reddish light.
And then it is best to forget about the constellations of the
zodiac, and simply look direct to the east. Most of you probably know
the constellation of the Big Dipper, which is, on these evenings, easy
to find not far from the zenith. Its “handle” points to a bright
orange star Arcturus. Actually, you do not need any assistance in
locating Arcturus. Just find the brightest star that is very nearly
overhead – if you look at about 9:30 or so. Later on, about midnight,
Arcturus will slowly slip to the west, and will be replaced at the
zenith by an even brighter star, Vega in Lyra, which has a bluish
color.
So here we have a nice collection of five bright stars. Each of
them represents a different type, and each of them lies at a different
distance from us. Nearest to us is Vega, but even this star is pretty
far by our terrestrial standards, 25 light years away. Arcturus comes
next with 34 light years, then Regulus at 72, and the two stars that
are most distant among these, Spica and Antares, shine at us from a
distance of about 142 light years. Imagine that the rays you will be
seeing now left the two stars in about 1860! Do you remember what
happened in your country and among your ancestors at that time?
Naturally, the two most distant stars among the bright ones must
actually be very luminous – yet for a different reason! Antares has a
cooler surface than our Sun, so each square inch of it emits less
light – but this is more than compensated for by the fact that Antares
is a supergiant star, with a radius about 700 times the radius of the
Sun. Spica competes very well with Antares as to its actual
brightness, in fact, it is more luminous – emits as much radiation as
some 6,300 Suns. This is due to its much higher surface temperature,
not to its much larger size, which is “only” about 8 times the size of
the Sun. |
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