© Jacek Halicki 2016. Perseid meteor seen in 2016 from Poland.

Leonid meteor shower

Dominic Ford, Editor
From the Meteor Showers feed

Please wait
Loading 0/4
Click and drag to rotate
Mouse wheel to zoom in/out
Touch with mouse to dismiss
The sky at

The Leonid meteor shower will be active from 6 November to 30 November, producing its peak rate of meteors around 17 November.

Over this period, there will be a chance of seeing Leonid meteors whenever the shower's radiant point – in the constellation Leo – is above the horizon, with the number of visible meteors increasing the higher the radiant point is in the sky.

Seen from Cambridge , the shower will not be visible before around 22:32 each night, when its radiant point rises above your eastern horizon. It will then remain active until dawn breaks around 06:07. The radiant point culminates (is highest in the sky) after dawn – at around 06:00 EST – and so the shower is likely produce its best displays shortly before dawn, when its radiant point is highest.

At this time, the Earth's rotation turns Cambridge to face optimally towards the direction of the incoming meteors, maximising the number that rain vertically downwards, producing short trails close to the radiant point. At other times, there will be fewer meteors burning up over Cambridge, but those that do will tend to enter the atmosphere at an oblique angle, producing long-lived meteors that may traverse a wide area of the sky before completely burning up.

The shower is expected to reach peak activity at around 18:00 EST on 17 November 2014, and so the best displays might be seen after the radiant rises on 17 November.

Begin typing the name of a town near to you, and then select the town from the list of options which appear below.

Observing prospects

At its peak, the shower is expected to produce a nominal rate of around 15 meteors per hour (ZHR). However, this zenithal hourly rate is calculated assuming a perfectly dark sky and that the radiant of the shower is situated directly overhead. In practice, any real observing sight will fall short of these ideal conditions. The number of meteors you are likely to see is thus lower than this, and can be estimated using the ZHR formula.

From Cambridge, the radiant of the shower will appear at a peak altitude of 69° above your horizon, and on the basis of this, we estimate that you may be able to see up to 14 meteors per hour at the shower's peak.

The shower will peak close to new moon, and so moonlight will present minimal interference.

The radiant of the shower

Meteor showers arise when the Earth passes through streams of debris left in the wake of comets and asteroids. Over time, these pieces of grit-like debris distribute themselves along the length of the parent object's orbit around the solar system.

Shooting stars are seen whenever one of these pieces of debris collides with the Earth, typically burning up at an altitude of around 70 to 100 km, upon impact with the upper atmosphere.

On certain days of the year, the Earth's orbit passes through particularly dense streams, associated with comets or asteroids which have vented particularly large amounts of solid material to space, and this gives rise to an annual meteor shower. The shower recurs on an annual basis, whenever the Earth passes the particular point in its orbit where it crosses the stream of material.

All of the meteors associated with any particular meteor shower appear to radiate outwards from a common point on the sky, which points back in the direction from which their orbital motion brought them.

This is because all the meteors are travelling in almost exactly the same direction when they cross the Earth's orbit, owing to having very similar orbits to the parent object they came from. They strike the Earth from almost exactly the same direction, and at the same speed.

By determining the position of this radiant point on the sky, it is possible to work out the orbit of the stream giving rise to any particular meteor shower. It is sometimes even be possible to identify the particular body responsible for creating the debris stream, if there is a known comet or asteroid with a very similar orbit.

The parent body responsible for creating the Leonid shower is comet 55P/Tempel-Tuttle.

The radiant of the Leonid meteor shower is at around right ascension 10h00m, declination 22°N, as shown by the green circle on the planetarium above.

To see the most meteors, the best place to look is not directly at the radiant itself, but at any dark patch of sky which is around 30–40° away from it. It is at around this distance from the radiant that the most meteors will be seen.

?>
The sky on 17 November 2014
Sunrise
06:36
Sunset
16:20
Twilight ends
17:57
Twilight begins
04:59

25-day old moon
Waning Crescent

19%

25 days old

Planets
Rise Culm. Set
Mercury 05:34 10:42 15:50
Venus 07:07 11:53 16:38
Moon 01:39 07:41 13:43
Mars 10:41 15:10 19:38
Jupiter 22:32 05:35 12:35
Saturn 06:35 11:32 16:30
All times shown in EST.

Source

The International Meteor Organisation's List of Meteor Showers.

Image credit

© Jacek Halicki 2016. Perseid meteor seen in 2016 from Poland.

Cambridge

Latitude:
Longitude:
Timezone:

42.38°N
71.11°W
EDT

Color scheme