Over the coming months the planets Mars, Jupiter, and Saturn will start to make an appearance in the evening sky. Jupiter is the first planet to make an appearance in the evening sky and is the subject of this article.
Jupiter image made by Hubble Telescope April 7, 2017. Image Credits: NASA, ESA, and A. Simon (NASA Goddard)
Jupiter’s Opposition arrives on May 9, this year, which is the point the earth is on a line between it and the sun. This time is also the best time to view the planet as it is closest to earth and is also in a favorable position of the sky for viewing. However, great views of Jupiter can be had now as it’s beginning to rise in the late evening. Look for a brilliant star rising in the east around 10 pm.
As usual, this article contains a lot of my own material since I actually get out there and observe astronomical objects!
Finding Jupiter is not difficult because it looks like a brilliant star and it is just a matter of knowing when it rises. Like all planets and stars, Jupiter always rises in the east (it could be Southeast or Northeast depending on where you live).
From data obtained by US Naval Observatory I was able to generate this plot of rising and transit times of Jupiter. Transit time occurs when the planet is highest in the sky and is typically when the best views are obtained. Although the graph has been done for a latitude of 35 North it should be approximate for most other locations.
Rise and Transit times for Jupiter. For example on May 25, 2018, Jupiter will rise at 6:15 pm, and will be highest in the sky around 11:40 pm
Jupiter is the largest of all the planet's in our solar system with a mean diameter of 140,000 km or 11 times larger than earth's diameter. Because the planet rotates so fast it's equator stretches out making it noticeably oblate. One full rotation on Jupiter takes just 10 hours. The following image shows the various structures of the planet nicely.
A cross section of Jupiter. Image Credit: Kelvinsong via Wikimedia Commons
Hydrogen and Helium are the primary constituent elements of Jupiter. However, the atmospheric layer visible to earth contains a perpetual layer of clouds made of Ammonia mixed with various chromophores. The composition of the chromophores is unknown but possibly include compounds of Phosphorus, Sulphur, as well as Hydrocarbons.
A probe dropping down into Jupiter's Atmosphere will not encounter a solid surface. Instead, increasing pressure results in the predominately Hydrogen becoming a supercritical liquid where it's liquid and gas phases are indistinct. For a demonstration of supercritical gases see this fascinating video.
Further down into Jupiter the pressure becomes so high that Hydrogen forms an exotic state called Metallic Hydrogen. In this form of Hydrogen, the electrons are squeezed out of the atoms and are free to conduct electricity which in turn helps power Jupiter's powerful magnetic field.
Jupiter looks like a brilliant star to the naked eye. However, even with binoculars, the planet begins to show as a small disk surrounded by 4 bright moons.
I've already written a series of articles on the moons of Jupiter. Check out the following:
But to summarise, there are at least 69 known moons of Jupiter, although only 4 (Galilean) moons are large. The Galilean moons include Io, Europa, Ganymede, and Callisto. These moons look like a string of stars set in a line next to Jupiter, similiar to the following image.
The moon, Jupiter and the Galilean moons. Photographed with a 200mm f4 lens and OMD-EM5 on a tripod. The exposure is about 1 second
Jupiter has a complex cloud belt layer that sits at the top of its atmosphere. Through a small telescope, Jupiter usually appears to have 2 dark belts that run across its disk. These are called the North and South Equatorial Belts. The Belts are darker primarily because of the relative transparency of the higher cloud decks in those areas that expose darker regions lower in the atmosphere. Here is an image of Jupiter (next to the moon) which is indicative of how Jupiter looks in a small telescope at low magnification.
Jupiter (center) appears near the limb of the moon in this view from the afternoon of June 16, 2005. This is very similiar to the view in a small telescope at low magnification. Note there is a vague indication of the 2 equatorial belts across the planet
At higher magnification, much more detail becomes visible in Jupiter's disk. In an average size amateur telescope at about 200x magnification, the view is very similar to the following image. The North and South Equatorial belts are now prominent, and there are subtle indications of other belts.
This view of Jupiter is similiar to what it looks like at approximately 200x magnification in an amateur telescope under typical sky conditions
Viewing Jupiter in a high-quality telescope when atmospheric conditions are excellent is an experience not soon forgotten. The belts no longer appear uniform but show intricate festoons and swirls. Subtle color differences are now apparent with a range of purples, orange and creme hues. The following image is indicative of the view of Jupiter under these circumstances.
This view of Jupiter is similiar to what it looks like at approximately 500x magnification in a high quality amateur telescope under excellent sky conditions
With modern cameras and new processing software very small details can be seen on Jupiter. The following animated gif was from March 17, 2018, while testing a new Monochrome camera and shows the rapid rotation of Jupiter over a period of 15 minutes in addition to the cloud detail. The camera used for this was a QHY183M and the telescope a Celestron C14.
Jupiter image over a 15 minute period on March 17, 2018. Note the planet's
rotation is plainly visible as well as the great red spot on the right hand
limb of the planet
The Juno Spacecraft recently returned some striking views of Jupiter. Looking through some of the images I was keen to find an image showing some 3D aspect of the cloud tops. I think this image fits the bill.
Jupiter’s northern polar belt region. Image credit:NASA/JPL-Caltech/SwRI/MSSS/ Björn Jónsson
The Great Red Spot (GRS) is one of the coolest features of Jupiter and has been around as long as the telescope has existed. These days, the red is a bit washed out so it doesn't quite stand out as much as it used to and when seen through a telescope reminds one of an eye. Here is an image I managed a while back showing the great red spot, which shows the sort of image you can get using an amateur telescope.
Jupiter with the Great Red Spot using a C14 Telescope and QHY183c camera
The cause of the GRS was unknown until the first space probes arrived at Jupiter and reveal it to be an enormous hurricane large enough to engulf the earth. Even though it has shrunk in recent decades it is still larger than the earth. The GRS's cyclonic nature is clearly visible in this remarkable movie made by Voyager 1 as it approached Jupiter.
Voyager 1 footage of Jupiter over the period of
a month. Image Credit: NASA/JPL
One of the less expected features you might see on Jupiter is an impact scar caused by an asteroid or comet colliding with the planet. Although rare, they have been observed several times in the past few decades. The impact of Comet Shoemaker-Levy in 1994 with Jupiter is one of the most amazing things I've ever witnessed. Perhaps this year we may witness another.
Over the next few months look for Jupiter in the eastern sky during the evening. To the naked eye it is easy to identify as a brilliant star, but as discussed above even a small telescope will reveal many interesting details including some of its moons and the planet's dynamic cloud belts.
One of the best places for information for Jupiter is the actual space mission websites. Here are some example sites you might want to visit.
| Mission | URL |
|---|---|
| Voyager 1 and 2 | https://photojournal.jpl.nasa.gov/mission/Voyager |
| Galileo | https://photojournal.jpl.nasa.gov/mission/Galileo |
| Juno | https://www.nasa.gov/mission_pages/juno/main/index.html |
For accurate rise/set times for your own location check out the US Naval Observatory web site.
NOTE: All images are the author's unless otherwise specified
