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η-Lyrid meteor shower

Dominic Ford, Editor
From the Meteor Showers feed

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The sky at

The η-Lyrid meteor shower will be active from 3 May to 14 May, producing its peak rate of meteors around 8 May.

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

From Seattle the radiant point is circumpolar, which means it is always above the horizon and the shower will be active throughout the night.

The radiant point culminates (is highest in the sky) after dawn – at around 05:00 PDT – 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 Seattle 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 Seattle, 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 15:00 PDT on 8 May 2018.

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Observing prospects

At its peak, the shower is expected to produce a nominal rate of around 3 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 Seattle, the radiant of the shower will appear at a peak altitude of 86° above your horizon, and on the basis of this, we estimate that you may be able to see up to 2 meteors per hour at the shower's peak.

The Moon, in Capricornus, will be around last quarter phase at the shower's peak, presenting minimal interference.

The origin of the shower

Meteor showers arise when the Earth passes through streams of debris left behind in the wake of comets and asteroids. Over time, the pieces of grit-like debris in these streams 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's atmosphere, typically burning up at an altitude of around 70 to 100 km.

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. Such showers recur on an annual basis, whenever the Earth passes the particular point in its orbit where it crosses the particular stream of material.

The geometry of meteor shower radiants The geometry of meteor shower radiants
All of the meteors associated with any particular shower appear to radiate from a common point on the sky.

The meteors that are associated with any particular meteor shower can be distinguished from others because their paths 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 the grit particles in any particular stream 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.

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.

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 η-Lyrid shower has been identified as comet C/1983 H1 (IRAS-Araki-Alcock).

The radiant of the η-Lyrid meteor shower is at around right ascension 19h00m, declination 44°N, as shown by the green circle on the planetarium above.

The sky on 08 May 2018
Sunrise
05:41
Sunset
20:30
Twilight ends
22:45
Twilight begins
03:26

22-day old moon
Waning Crescent

39%

22 days old

Planets
Rise Culm. Set
Mercury 05:02 11:33 18:03
Venus 07:05 15:06 23:07
Moon 02:55 07:49 12:44
Mars 01:44 06:01 10:17
Jupiter 20:15 01:10 06:00
Saturn 00:25 04:42 08:59
All times shown in PDT.

Source

The position of the radiant of this shower, and its predicted hourly rate, were taken from International Meteor Organisation's List of Meteor Showers.

Image credit

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Seattle

Latitude:
Longitude:
Timezone:

47.61°N
122.33°W
PDT

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