…Record the Geminid meteor shower.
December’s cold and frosty nights mark the arrival of the year’s richest meteor showers: the Geminids. The shower runs from 8-17 December with peak activity occurring on the morning of 14 December. This year the Moon sets before 21:30 UT so the display won’t be drowned in lunar glare. Here, we’re going to look at why these observations are useful to researchers and how best to observe the Geminids and record them.
All meteor showers are produced by either a comet or an asteroid that we call the parental body. The Geminids are caused by 3200 Phaethon, an Apollo-type asteroid that orbits the Sun every 1.4 years. 3200 Phaethon has a rather eccentric orbit; the furthest it ever gets from the Sun is a distance of 2.4 AU (aphelion) but its closest distance (perihelion) is just 0.1AU – closer to the Sun than the planet Mercury. 3200 Phaethon has the distinction of being the only asteroid in the Solar System to get this close to the Sun!
While it’s in the inner Solar System, heat from the Sun causes particles to escape from the surface of Phaethon and fly away into space. Eventually, these particles collide with Earth; they burn up as they hit the atmosphere, causing a glowing trail, or what we call a meteor or ‘shooting star’.
Since Earth is colliding with a cloud of particles, the meteors appear to us to come from one direction in the sky; this is called
the radiant and the location of the radiant gives the name of the shower. The radiant for meteors in the constellation of Gemini gives the shower its name: the Geminids.
Meteor showers are a good opportunity for astronomers to study their parental bodies, so amateur observations are
particularly welcomed by organisations such as the British Astronomical Association (BAA). If, for example, analysis of the observations reveals that the radiant has shifted, this could indicate orbital changes. We can also infer how active the parental object has been during its passage into the inner Solar System.
Make it a group activity
Useful observations of meteors require an organised meteor watch. You can look for meteors on your own, but it is common to observe in groups with one member acting as a recorder and filling in the form as the various observers call out their sightings. The report form used by the BAA is available electronically, so you can print it out and use it during your session.
Although the Geminids have a Zenithal Hourly Rate (ZHR) of over 100 meteors an hour, this number can be misleading since it assumes optimum viewing conditions: a radiant that’s high in the sky and no light pollution or clouds. In reality you won’t see as many as this. Geminids tend to be swift and usually white in colour – the streak they leave behind is called a meteor train and it may persist for a few seconds.
You’ll need to record the names of all observers, your location and contact details along with the start and end times (in UT) of your session. You also need to make a note of the stellar limiting magnitude of your site by locating and identifying the faintest star you can see with the naked eye.
As the watch gets underway, you’ll need to record the times the meteors were observed along with their estimated magnitude. Remember, not all of the meteors observed will be Geminids! A true Geminid will have either a short train close to the radiant or a longer one further away; it must also be moving away from the radiant. If your meteor is not obeying these rules it is what’s known as a ‘sporadic’ and not part of the shower – you should still record it but label it ‘sporadic’. You also need to include any constellations that the meteor passes and how long it takes to fade.
Once indoors, you should type your observations into the report form and save it on your computer so that you have a good permanent record. And don’t just let the data you’ve collected sit around. Send your observations to the Meteor Section of the BAA – the scientists there will make good use of the data!
The further away a meteor appears from the radiant of the shower, the longer its trail will be