Astronomy - 06.2019

(John Hannent) #1
BINOCULARUNIVERSE
BY PHIL HARRINGTON


N

E

ARIES

CETUS

TAURUS

Path of Vesta

Oct 21
31
Nov 10
20 30 Dec^10

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j
k h


OPHIUCHUS

SCORPIUS

LIBRA

q e

r

t

i

`

t
t

b

h

Path of Ceres

May 12 22
June 1 11
21
July 1

11
21

31

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14 ASTRONOMY • JUNE 2019

O


n January 1, 1801,
Italian astrono-
mer Giuseppe
Piazzi spotted a
“star” through his
telescope that was not on his
detailed charts of the region. He
returned to the same location
over the next few nights, only to
find that this new star couldn’t
be a star at all. It had moved
against the stationary backdrop.
Whatever he had discovered, it
had to be orbiting the Sun.
At first, he thought he had
discovered a comet, but later
observations (by him and oth-
ers) allowed an orbit to be cal-
culated. Piazzi’s new object was
revolving around the Sun in a
nearly circular orbit at a dis-
tance of 2.77 astronomical
units. (An AU is the average
Earth-Sun distance.) That
placed it in the gulf between
Mars and Jupiter. He had dis-
covered the first asteroid, now
reclassified as a dwarf planet by
the International Astronomical
Union. As is customary, the
discoverer of a new member of
the solar system has the honor
of naming it. Piazzi chose

Ceres for the Roman and
Sicilian goddess of grain.
Asteroids can change dra-
matically in brightness depend-
ing on their distance from
Earth. The best time to look for
them is when their distance
away from us is minimal. This
occurs at opposition, when the
asteroid rises in the east as the
Sun sets in the west.
June opens with Ceres just
past its May 28 opposition.
From late May through early
July, it appears to move in ret-
rograde as quicker Earth passes
by. During this time, it slides
from Ophiuchus, through
northernmost Scorpius, and
into Libra. Throughout, it will
remain around 7th magnitude.
Of course, that region of the
sky has lots of 7th-magnitude
stars, so spotting which one is
Ceres is a bit like looking for a
celestial needle in a haystack.
Ceres moves past several
notable stars during the month,
which should help in our quest.
I hope the sky is clear for you
May 24 and 25. On those
nights, Ceres is just north
of 4th-magnitude Chi (χ)

Ophiuchi. As it continues to
march westward, it passes 1.5°
north of 4th-magnitude Nu (ν)
Scorpii on June 9, and on the
17th, it appears 1.6° north of
Graffias (Beta [β] Scorpii).
During July, its retrograde
motion will slow, allowing
Ceres to resume its normal,
easterly track. It will hover
between Graffias and Lambda
(λ) Librae, slowly arcing south,
then southeast by the end of the
month. In the process, Ceres
will fade by more than a magni-
tude since June 1.
Once you spot Ceres, make
visiting it a habit over the next
few months. Note its position
on the chart each time you
glimpse it. In the end, you’ll
have a personal record of Ceres’
2019 apparition.
Ceres is not the only member
of the asteroid belt visible
through your binoculars. More
than 60 become brighter than
10th magnitude around opposi-
tion, and should therefore be
visible through binoculars.
On August 13, the 15th aster-
oid discovered, Eunomia, will
reach opposition. That night, it
will shine at magnitude 8.2,
faint but doable through
steadily supported 50mm bin-
oculars. It will lie among the
faint stars of Aquarius, 3.7° west
of Sadalsuud [Beta Aquarii].
You’ll need a good finder chart
to locate this challenging target.
(More on that later.)
Surprisingly, even though
Ceres is the largest object in the
asteroid belt at about 600 miles
(960 kilometers) across, it is not
the brightest. That honor goes

to Vesta, the fourth asteroid
discovered. German physician
Heinrich Olbers found Vesta on
March 29, 1807. Olbers had also
discovered the asteroid Pallas
five years earlier.
Vesta always puts on a fine
show around opposition. That’s
next set to occur November 12.
At that time, Vesta will be
within the constellation Cetus
the Whale. At opposition, Vesta
will be 1.56 AU from Earth and
shine at magnitude 6.5. It will
be 1.9° west-southwest of 4th-
magnitude Omicron (ο) Tauri,
which marks one of the Bull’s
front hoofs. That night’s Full
Moon will be only about a bin-
ocular field away, confounding
efforts to see Vesta. But take
heart. Vesta stays bright several
weeks before and after opposi-
tion: In November, it remains
brighter than 7th magnitude
and within binocular range.
I mentioned earlier that
Eunomia would be challenging
to search for, and the same is
true of most asteroids — accu-
rate finder charts are a must.
One of the best online resources
for this is in-the-sky.org/
newsindex.php?feed=asteroids.
Good luck with this introduc-
tion to asteroiding.
I’d enjoy hearing your
results. Contact me through my
website, philharrington.net.
Until next month, remember
that two eyes are better than
one.

Let’s go


asteroiding!


Minor planets make for challenging binocular targets.
Ceres crosses into Ophiuchus, Scorpius, and Libra from late May through early July.

Vesta remains bright weeks before and after the asteroid’s opposition November 12.

Phil Harrington is a longtime
contributor to Astronomy and
ASTRONOMY the author of many books.

: ROEN KELLY

ASTRONOMY

: ROEN KELLY
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