NASA Comments on a Supermoon Event Happening on September 28th
During lunar perigee, the moon appears larger and brighter in the sky, which is why a full moon coinciding with perigee is known as a “supermoon”. “On September 27, we’re going to have a perigee full moon – the nearest full moon of the year”, Petro included.
The officials said that the regions from where a total lunar eclipse will be seen are North America, western Asia, South America, Europe, eastern Pacific Ocean and Africa.
As seen from the moon, the Earth hides the Sunday .
“Since the moon’s circle is not a flawless circle, the moon is now and again closer to the Earth than at different times amid its circle”, Noah Petro, agent venture researcher for the Lunar Reconnaissance Orbiter at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, said in an announcement. This is the super moon shadow, and it begins to look awesome because it is getting ready to undergo a total eclipse, which we will be able to see. That distance equates to a few times around the circumference of Earth.
A super moon occurs when the moon will look bigger and brighter than usual since it will be at its closest approach to the earth as it makes its orbit. The Slooh Community Observatory, a skywatching website that provides users access to remotely operated telescopes, will offer a flagship webcast of the lunar eclipse that can be accessed at the Slooh website, where visitors can also find Slooh’s archive of past webcasts.
In contrast, lunar eclipses are quite popular, occurring two times a year at the least. A lunar eclipse occurs about twice per year when the earth is situated when our planet blocks the sun’s rays from illuminating the moon (image below from Earth Sky).
Several webcasts are planned to stream live views of the eclipse online. When the total lunar eclipse takes place, it will cover the moon’s face. Earth’s shadow will begin to dim the supermoon slightly beginning at 8:11 p.m. EDT. After September 27, the next phenomenon of this sort will take place in 2033.