Latest Posts by frankielazalde - Page 5

Lovely cat

Foot

Vas a salir de ésta y de muchas más. Atte: La Muerte.

Ternuringas

Friendship Goals

L&R

Moon

Gato.

El faro de la casa.

Momentos que se pierden como lágrimas.

Calavera

El gato y el láser.

People.

El gato

Subtle Lunar Eclipse

Today’s (Feb. 10) lunar activity comes in the form of a penumbral eclipse. What does that mean and how does this type differ from a total eclipse? Let’s take a look:

First off, what is a penumbra? During a lunar eclipse, two shadows are cast by the Earth. The first is called the umbra (UM bruh). This shadow gets smaller as it goes away from the Earth. It is the dark center of the eclipse shadow where the moon is completely in the shadow of the Earth.

The second shadow is called the penumbra (pe NUM bruh). The penumbra gets larger as it goes away from the Earth. The penumbra is the weak or pale part of the shadow. This occurs because the Earth is covering a portion of the sun.

Penumbral eclipses occur when only the outer shadow (the penumbra) of Earth falls on the moon’s surface. This type of eclipse is much more difficult to observe than total eclipses or when a portion of the moon passes into the umbra. That said, if you’re very observant, you may notice a dark shadow on the moon during mid-eclipse on Friday evening. You may not notice anything at all. It’s likely the moon will just look at little bit darker than normal…like this: 

Earth’s penumbral shadow forms a diverging cone that expands into space in the opposite direction of the sun. From within this zone, Earth blocks part but not the entire disk of the sun. Thus, some fraction of the sun’s direct rays continues to reach the most deeply eclipsed parts of the moon during a penumbral eclipse.

For most of North America, the penumbral eclipse will begin at moonrise (sunset) on Friday, Feb. 10 and will be obscured by evening light. Here’s a guide of when to look up:

Fun fact: Aristotle (384 – 322 BCE) first proved that Earth was round using the curved umbral shadow seen at partial eclipses. In comparing observations of several eclipses, he noted that Earth’s shadow was round no matter where the eclipse took place. Aristotle correctly reasoned that only a sphere casts a round shadow from every angle.

To learn more about lunar eclipses, visit: https://svs.gsfc.nasa.gov/11828

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

Entre más arriba estas, más lento corre el tiempo.

Querrás bajar, pero ya todo habrá cambiado.