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Posted by MFish • Profile • 07/14/21 at 11:45PM • Life Stories - Memories • See more by MFish

I search my mind.
I scratch and scribe,
upon the paper,
using my old hand,
as I pull forth,
some words, from out
the brackish water, mine.
I wish you well,
for now's the day,
to change your life,
while you are still
the wife I know,
who lives in this house,
morning, noon and night.
Stay close to me
for the care givers life,
is never over or done.

NASA Astronomy Picture of the Day:

What happens when a black hole destroys a neutron star? Analyses indicate that just such an event created gravitational wave event GW200115, detected in 2020 January by LIGO and Virgo observatories. To better understand the unusual event, the featured visualization was created from a computer simulation. The visualization video starts with the black hole (about 6 times the Sun's mass) and neutron star (about 1.5 times the Sun's mass) circling each other, together emitting an increasing amount of gravitational radiation. The picturesque pattern of gravitational wave emission is shown in blue. The duo spiral together increasingly fast until the neutron star becomes completely absorbed by the black hole. Since the neutron star did not break apart during the collision, little light escaped -- which matches the lack of an observed optical counterpart. The remaining black hole rings briefly, and as that dies down so do the emitted gravitational waves. The 30-second time-lapse video may seem short, but it actually lasts about 1000 times longer than the real merger event. Astrophysicists: Browse 2,500+ codes in the Astrophysics Source Code Library

Do you remember
the hoot of an Owl?
Or the sound of breaking glass
when wrapped in a towel?
Unlike the Owl,
who calls out my name
of all the new pain
of losing your memories,
all over; once again.
The caw of the Crow
when it's time for a feed,
is all they want and need.
A songbird now sings
in a tree, over there,
a pleasant sound in the Summer air.

NASA Astronomy Picture of the Day:

What has happened to Saturn's moon Iapetus? Vast sections of this strange world are dark brown, while others are as bright white. The composition of the dark material is unknown, but infrared spectra indicate that it possibly contains some dark form of carbon. Iapetus also has an unusual equatorial ridge that makes it appear like a walnut. To help better understand this seemingly painted moon, NASA directed the robotic Cassini spacecraft orbiting Saturn to swoop within 2,000 kilometers in 2007. Iapetus is pictured here in 3D. A huge impact crater seen in the south spans a tremendous 450 kilometers and appears superposed on an older crater of similar size. The dark material is seen increasingly coating the easternmost part of Iapetus, darkening craters and highlands alike. Close inspection indicates that the dark coating typically faces the moon's equator and is less than a meter thick. A leading hypothesis is that the dark material is mostly dirt leftover when relatively warm but dirty ice sublimates. An initial coating of dark material may have been effectively painted on by the accretion of meteor-liberated debris from other moons.

The wayward Sun, is like our Son,
full of music with a dose of passion,
for he has always been a guitar man.
An acoustical one, playing in his fashion.
Progressive Rock and Roll he says he plays.
Spending studio time to create a CD Action.
His musical talent, as he plays his songs,
brings forth a noise; to me a distraction,
but he loves it so, he will play
as his band becomes the latest music attraction.

NASA Astronomy Picture of the Day:

What will become of our Sun? The first hint of our Sun's future was discovered inadvertently in 1764. At that time, Charles Messier was compiling a list of diffuse objects not to be confused with comets. The 27th object on Messier's list, now known as M27 or the Dumbbell Nebula, is a planetary nebula, one of the brightest planetary nebulae on the sky -- and visible toward the constellation of the Fox (Vulpecula) with binoculars. It takes light about 1000 years to reach us from M27, featured here in colors emitted by hydrogen and oxygen. We now know that in about 6 billion years, our Sun will shed its outer gases into a planetary nebula like M27, while its remaining center will become an X-ray hot white dwarf star. Understanding the physics and significance of M27 was well beyond 18th century science, though. Even today, many things remain mysterious about planetary nebulas, including how their intricate shapes are created.

Photo by Bray FallsKeith Quattrocchi

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