Planet Adventures In The Sky

Sometimes a whole bunch of different sky events happen over a very short period, giving skywatchers a chance to witness many unusual events in a few days. The next week or two is a case in point.

Uranus at opposition

First, the planet Uranus is just past opposition, so it is visible all night long. It’s also in a location where you can spot its dim glow rather easily. You will need a binocular to bring out the faint planet from its surrounding stars

Look at the chart above, and you will see how to spot Uranus using an easy bit of star hopping.

Start with visualizing an equilateral triangle with one side marked by Hamal in Aries and Algenib, the lower left star of the square of Pegasus. The third point of the triangle is Alrescha, Alpha Piscium.

Although only fourth magnitude, Alrescha is the second brightest star in the dim constellation of Pisces. It marks the knot which joins the two chains of stars attached to the two fish of Pisces. Follow the lower chain of stars to the right under the square of Pegasus to find Uranus.

The stars that make up this chain do not have names, only Greek letters. Starting at Alrescha, they are Nu, Mu, Zeta, and Epsilon. You don’t need to know their names, just look for Uranus between the last two, a bit to the south of the line joining them. 

In binoculars, Uranus will look like a blue green 6th magnitude star. In a powerful telescope, it will show as a tiny blue-green disk 3.7 arc seconds in diameter.

Arc seconds

Planetary diameters are usually measured in arc seconds: the number of seconds they subtend at the observer’s eye. There are 360 degrees in a circle, 60 minutes in a degree, and 60 seconds in a minute. To give you some idea how tiny the planets appear, the sun and moon are both around 30 arc minutes in diameter, or 1800 arc seconds. The largest any planet can appear to Earthbound astronomers is Venus at its closest, which is about 1 arc minute or 60 arc seconds in diameter. Thus all the planets are typically smaller in a telescope than the largest craters on the moon. 

Mercury at greatest elongation

On Thursday, October 15, Mercury will be at the farthest it strays west of the sun. Because it is only 18 degrees away from the sun, it can best be seen about half an hour before sunrise. Again it is easiest to spot in binoculars. It is about twice the angular diameter of Uranus, so will look like a tiny half moon 8 arc seconds across in a large telescope.

Mars near Jupiter

On Sunday morning, October 18, Mars will be in conjunction with Jupiter, and the two planets will be close enough together that both will fit in the same field of a small telescope. Look for Mars just above Jupiter.  

Both will be on the far side of the Sun, so much smaller than they usually appear when in the evening sky. Jupiter measures 32 arc seconds while Mars is only 4.1 arc seconds, half the size of Mercury. By the time they reach opposition in spring of 2016, they will swell to 44 and 18.3 arc seconds respectively.

Double shadow transits on Jupiter 

Speaking of Jupiter, there will be two interesting passages of the shadows of its moons across its face in the next two weeks. These require at least a 5-inch telescope and steady observing conditions.

Again on Sunday morning, October 18, the shadow of the moon Io will chase the shadow of Ganymede across Jupiter’s face. Both shadows will be on Jupiter from 6:42 to 8:08 a.m. EDT, but will be increasingly hard to see after sunrise at around 7:30 a.m. local time. Observers in western parts of North America will have a better view because the transits will occur between 3:42 and 5:08 a.m. PDT, long before sunrise, though Jupiter will be lower in the sky.

Exactly a week later. on Sunday October 25, there will be another double shadow transit. This one is especially interesting because both shadows enter the disk at almost the same time, 8:36 a.m. EDT or 5:36 a.m. PDT, but then cross at very different speeds, Io’s shadow taking 2 hours and 17 minutes to cross while Ganymede’s takes 3 and a half hours, because of its greater distance from Jupiter and larger orbit diameter.

This transit occurs in full daylight in eastern North America, so probably won’t be visible, but is at a much more favorable time for western observers.

All in all, planetary observers will have a busy week ahead and, as always, we welcome your images of these events.

Mars Visits the Beehive Star Cluster

Considering the thousands of stars in the sky, it is surprisingly rare to see a star in the same telescope field as one of the planets. The reason is that planets generally require a lot of magnification, and this severely limits the field of view of a telescope when looking at a planet.

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On Thursday morning, August 20, just before dawn, the planet Mars will pose in front of a swarm of stellar bees, the Beehive Cluster (Messier 44) in the constellation Cancer. Credit: Starry Night software.

On the morning of Thursday, August 20, we will get a special treat, when the planet Mars appears in the midst of hundreds of stars: the open star cluster known as the Beehive, Praesepe, or Messier 44.

This star cluster is called “the Beehive” because of its resemblance to a swarm of bees. It is also known as “Praesepe,” which is Latin for “manger,” because of its position between the stars Asellus Borealis and Asellus Australis, the northern and southern donkeys. Finally, it is number 44 in Charles Messier’s famous catalog of deep sky objects.

Located 590 light years from the sun, the Beehive is one of the nearest and brightest star clusters in the sky. Its several hundred stars are concentrated in a volume 16 light years across, and it actually outshines all of the individual stars in its constellation, Cancer.

You may be wondering where Mars is in the sky, because we haven’t heard much about it lately. That is because it has been on the far side of the sun in recent months, and impossible to see. It is only now emerging from the sun’s glare and reappearing in the morning sky, just before dawn. Look for it around 5 a.m. this week low in the northeastern sky, and be sure to use binoculars if you want to see the Beehive behind it.

Even in the smallest telescope, Mars should make a pretty picture lying in front of the many stars of the Beehive. But be sure to catch it Thursday or Friday morning, because by Saturday it will have passed the Beehive.

Mars itself will be a disappointing sight, as it is still very far away from Earth, 2.5 astronomical units distant and less than 4 arc seconds in diameter. It won’t be large enough to show much detail until mid-March next year, heading towards its most favorable opposition in over a decade