Astronomy - June 2015

(Jacob Rumans) #1

SOUTHERN


SKY


MARTIN GEORGE describes the solar system’s changing landscape
as it appears in Earth’s southern sky.

August 2015: Planets gather in evening


August begins with three
bright planets hanging low in
the western sky during evening
twilight. Venus, Jupiter, and
Mercury team up with the
1st-magnitude star Regulus to
create a fine binocular scene,
but don’t procrastinate — the
vista won’t last long.
Venus is the highest and
brightest of this group. It stands
at an altitude of 15° a half-hour
after sunset and shines bril-
liantly at magnitude –4.4. The
planet proves to be a captivating
sight when viewed through a
telescope. It appears more than
50" across and sports a razor-
thin crescent just 7 percent lit.
The planet’s large size makes
the crescent easy to see even
under the adverse seeing condi-
tions typical at low altitudes.
Venus disappears into the
twilight glow during August’s
second week as it prepares
to pass between the Sun and
Earth. (This so-called inferior
conjunction occurs on the
15th.) But the planet returns to
view before dawn barely a week
later. By the 31st, you can find
it about 10° above the eastern
horizon 30 minutes before sun-
rise. A telescope then shows
Ve nu s l o o k i n g r e m a r k a b l y
similar to the way it did at
the beginning of the month.
Jupiter behaves in much
the same way as Venus does
during August, but the outer
planet moves at a slower pace.
On the 1st, you can find Jupiter
6° to Venus’ lower right. Shin-
ing at magnitude –1.7, the giant
world appears prominent
despite glowing less than 10
percent as bright as its neigh-
bor. Unfortunately, poor seeing

conditions near the horizon
mean a telescope won’t show
much detail on the planet’s
31"-diameter disk.
The gas giant world appears
2° below Regulus on August 1.
As the gap between these two
objects closes during the fol-
lowing week, Mercury joins
the group. Pay particular atten-
tion from around August 5 to 7,
when the three objects appear
within 2° of one another and
Venus lies some 5° to their left.
For the best views, use binoc-
ulars and observe from a site
with an unobstructed view of
the western horizon.
Jupiter becomes lost in twi-
light within another week, pass-
ing on the far side of the Sun
from our viewpoint August 26.
Meanwhile, Mercury climbs
higher in the evening sky.
Although the innermost planet
won’t reach the peak of its appa-
rition until early September, it
becomes the most conspicuous
object in the western sky by late
August. On the 31st, Mercury
shines at magnitude 0.1 and
appears nearly 15° high a full
hour after sunset. You can find
it among the background stars
of Virgo, some 20° below that
constellation’s brightest star,
1st-magnitude Spica. When
viewed through a telescope on
August’s final evening, Mercury
appears 7" across and slightly
more than half-lit.
Wait for darkness to fall
before targeting the solar sys-
tem’s most beautiful planet.
Saturn then lies high in the
northwest and in perfect posi-
tion for viewing with your
naked eye, binoculars, or a tele-
scope. The ringed planet shines

at magnitude 0.5 against the
backdrop of eastern Libra, not
far from the brighter stars of
northern Scorpius. Saturn lies
about 5° from both Beta (β)
and Delta (δ) Scorpii, a pair
of 2nd-magnitude suns in the
Scorpion’s head.
The planet’s high altitude in
early evening should translate
into splendid views through a
telescope. Saturn displays a
disk that measures 17" across
the equator surrounded by a
ring system that spans 38" and
tilts 24° to our line of sight. The
planet’s shadow appears as a
dark wedge falling on the rings
behind the planet just off the
disk’s eastern limb. Also keep
an eye out for 8th-magnitude
Titan, Saturn’s biggest moon
and the second largest in the
solar system.
You might catch your first
glimpse of Mars in late August
as it begins a nearly two-year
apparition. The magnitude 1.8
Red Planet hangs just 5° high in
the east-northeast 30 minutes
before sunrise. Search for it
through binoculars some 10°
to Venus’ lower left.

The starry sky
One night in July 1778, French
astronomer Charles Messier
discovered a fuzzy patch
of light in the constellation
Sagittarius. He described it as
a “very faint nebula ... [that]
contains no star. Messier did
not realize he was viewing a
distant globular cluster, which
his telescope could not resolve
into individual stars.
We now know that M54
does not even belong to our
galaxy. In 1994, astronomers

discovered the Sagittarius
Dwarf Spheroidal Galaxy and
soon realized that M54 formed
a major part of it. This galaxy is
far smaller than the Milky Way
and already has started to col-
lide with our own. The globular
cluster currently lies about
86,000 light-years from Earth.
M54 lies among the stars of
Sagittarius’ prominent Teapot
asterism, a region that rides
high in the eastern sky after
darkness falls these August eve-
nings. The cluster stands some
1.5° west-southwest of magni-
tude 2.6 Zeta (ζ) Sagittarii. M54
glows at 8th magnitude and
shows up through 7x50 binocu-
lars. If you can’t find it through
a telescope right away, center
magnitude 3.6 Gamma (γ) Sgr
in your field. Then, enjoy the
naked-eye and binocular view
of the winter Milky Way for
precisely 49 minutes. At the
end of the wait, M54 will be
centered in the field of view.
Once you’ve found the glob-
ular, you’ll understand why
Messier could not resolve it.
You’ll likely need a 10-inch or
larger scope to see even a hint
of granulation. Still, it’s a thrill
to view an object that belongs
to another galaxy.
Just last year, astronomers
looked at the abundance of
lithium-7 in M54. Our galaxy
has a puzzlingly low amount
of this element, and some
researchers suggested that this
scarcity applied only to the
Milky Way. But studies of the
stars in M54 seem to show that
this is not the case. Scientists
now think that the lithium
shortfall may exist throughout
the cosmos.
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