The Seasonal Almanac: Events for April and May 1996

By Fred Schaaf
Published on April 1, 1996
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PHOTO: FOTOLIA/HANSENN
The most fascinating feature of rhododendrons is the temperature behavior of their leaves, which enables us to use them as natural thermometers. The greater the angle of uplift in the rhododendron leaves, the higher the temperature.

The Seasonal Almanac shares astronomical events in April and May 1996. Brilliant Venus will actually cast shadows in May.

The Seasonal Almanac: Events for May 1996

Venus is the brightest point of light in
the heavens. But this spectacular planet is fairly close to
the Sun in space and therefore always appears fairly close
to the Sun in our sky. We are lucky when Venus is visible
for more than an hour or two before sunrise or more than an
hour or two after sunset. And this spring we are luckiest
of all: in its eight-year cycle of recurring appearances,
this is the spring that Venus soars to its highest in the
evening sky. As April begins, the brilliant “evening star”
hangs halfway up the southwest sky at sunset and does not
itself sink below the horizon until about four hours later.

A bonus for Venus watchers occurs at the start of April. On
April 2 and 3, Venus is skimming right along the edge of
the loveliest of all star clusters, the Pleiades, or “Seven
Sisters,” cluster. Although the cluster is usually easy to
see with the naked eye, the brilliance of Venus may so
overwhelm its stars that we’ll need binoculars to spot them
plainly. The next few nights, no optical aid should be
required to view the wonderful little grouping of
sapphire-like stars being left behind by the peerless
diamond of Venus.

Venus is noticeably lower at sunset by early May, but to
make up for this, the planet gets even brighter. The
maximum brilliance of Venus is almost unbelievable,
especially as seen from a rural site, where Venus is even
capable of casting shadows in a very dark location. Try to
see how soon before sunset each day you can first glimpse
Venus. On days of deep-blue sky, the planet can even be
found in the middle of the day with the unaided eye!

The final weeks of May bring us the drama of Venus
appearing appreciably lower with each passing night. At the
start of May, Venus sets over three and a half hours after
the Sun, but by the end of the month, only about one hour
after. And if you have a small telescope or even a pair of
binoculars you can hold steady, there is another wonder of
Venus to behold: the changing phase of the planet. Venus is
a planet closer to the Sun than Earth is, and it displays
to us phases like the moon does (fully lit globe of Venus,
half-Venus, crescent Venus … ) Of course, normally you
need a fairly good telescope to detect these phases. But in
May, Venus is approaching unusually close to Earth (not
dangerously close, don’t worry!). So even binoculars may
show it as more of a long, skinny crescent than as the
simple point of light it looks like to the naked eye.

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