Dominic Ford, Editor
From the Meteor Showers feed
The π-Puppid meteor shower will be active from 15 April to 28 April, producing its peak rate of meteors around 24 April.
Over this period, there will be a chance of seeing π-Puppid meteors whenever the shower's radiant point – in the constellation Puppis – is above the horizon, with the number of visible meteors increasing the higher the radiant point is in the sky.
Seen from Ashburn , the shower will be active each day from dusk until around 20:49 when its radiant point sets below your western horizon. The radiant point culminates (is highest in the sky) before nightfall – at around 18:00 EDT – and so the shower is likely produce its best displays soon after dusk, when the radiant point is still as high as possible.
At this time, the Earth's rotation turns Ashburn 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 Ashburn, and they 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 01:00 EDT on 24 April 2019, and so the best displays might be seen before the radiant sets on 23 April and after dusk on 23 April.
At its peak, the shower is expected to produce a nominal rate of around 0 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 Ashburn, the radiant of the shower will appear at a peak altitude of 1° above your horizon, and on the basis of this, we estimate that you are only likely to see only around 0 meteors per hour, even at the shower's peak, since the radiant will be relatively low in the sky.
The Moon, in Ophiuchus, will be around last quarter phase at the shower's peak, presenting significant interference in the pre-dawn sky after it rises at 23:40. However, it will be well separated from the shower in the sky, rising no higher than 29° above the horizon and lying 109° away from the shower's radiant. If you select an observing site where it is possible to conceal the Moon behind a wall or other obstruction, it may be possible to preserve a reasonable degree of night vision.
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 π-Puppid shower is comet 26P/Grigg-Skjellerup.
The radiant of the π-Puppid meteor shower is at around right ascension 07h10m, declination 45°S, 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 24 April 2019|
19 days old
All times shown in EDT.
The International Meteor Organisation's List of Meteor Showers.
© Jacek Halicki 2016. Perseid meteor seen in 2016 from Poland.