PC: Space.com
This year’s Eta Aquarid meteor shower is reaching its maximum activity, and the skies at night are about to put on an interesting show for observers. For many, the notion of witnessing shooting stars seems rather straightforward; however, it all boils down to the timing of observation. The margin between seeing no meteors and seeing multiple ones is actually very small, and this is something everyone needs to keep in mind. Unfortunately, this year is not a good one for observing the shower, yet experts claim that it is still quite possible to see several of them if one knows exactly when it would be the most appropriate time to do so.
Eta Aquarid meteors tonight: What is the best time to see
The optimal viewing time for the Eta Aquarid meteor shower this night will be at dawn on May 6. This implies spending time outdoors for about two or three hours before dawn. During this window, the Earth rotates toward the path of the debris caused by Halley’s comet, increasing the possibility of seeing meteors. According to astronomers, as the night passes, the radiant of the meteor shower, which is situated in the Aquarius constellation, moves upward from the horizon. At dawn, it will be in a more favorable position for viewing, making more meteors observable. For this reason, late-night viewing is not as productive as viewing at dawn.
Eta Aquarid meteors: How to find the right spot
When attempting to observe meteors, one needs to pay attention to the section of the sky where meteors are expected to appear. The constellation of Aquarius is where the radiant of the Eta Aquarids occurs. This section appears in the eastern part of the sky during early mornings. But one does not need to focus on the exact position of the radiant. Indeed, meteors usually occur far from the radiant. According to experts, focusing on a spot approximately 30 to 40 degrees away from the radiant would result in a better observation.One should also find an area that is relatively darker than others. Any artificial lighting in the vicinity can make it difficult to view meteors. Furthermore, one should wait for their eyes to adapt to the darkness for around 15 to 20 minutes.
Why you may see fewer meteors despite peak timing
While the timing may work to your advantage, there are other variables that could affect visibility. The major obstacle in terms of seeing the shower this year would be the presence of a bright Moon. With an 84 percent illuminated waning gibbous Moon that will rise shortly after midnight and stay visible throughout the night, this factor adds even more light into the atmosphere, making it more difficult to see the fainter meteors. It is possible that the number of visible meteors would be reduced by this factor. While the Eta Aquarid meteor shower usually brings many meteors into view, those located in the north will only see a few.However, brighter meteors are likely to remain visible.
What viewers in the northern hemisphere should expect
This particular meteor shower appears to be more advantageous for those located in the southern hemisphere as compared to their counterparts in the northern hemisphere, especially owing to better visibility conditions in the southern parts. While an observer in the southern hemisphere may potentially spot up to 50 meteors per hour during the peak of the Eta Aquariid Meteor Shower, one in the northern hemisphere is more likely to see about 10 to 30 meteors per hour under optimal viewing conditions, depending on the bright Moon. However, it may still be fun and worthwhile for those who would like to watch the night sky.
The best meteor sightings may come just before sunrise
The ideal opportunity to view Eta Aquarids in their full glory tonight will be just before dawn on May 6th. This is the period when there will be the highest probability of viewing meteors, despite the lack of ideal circumstances. The Eta Aquarid meteor shower may not offer a steady stream of meteors, but it does have its special moments. All that one needs is a glimpse of a shooting star to get a memory of a lifetime. Go to Source
