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Still the Same

Posted by MFish • Profile • 08/23/24 at 11:20PM • Poetry • See more by MFish

Fighting insanity,
every day,
as my life,
slips away.

I feel good,
is what to know,
for my life is my
own traveling show.

How it will end
everyone will know
for I may well be
the next one to go.

NASA Astronomy Picture of the Day:

There is a quiet pulsar at the heart of CTA 1. The supernova remnant was discovered as a source of emission at radio wavelengths by astronomers in 1960 and since identified as the result of the death explosion of a massive star. But no radio pulses were detected from the expected pulsar, the rotating neutron star remnant of the massive star's collapsed core. Seen about 10,000 years after the initial supernova explosion, the interstellar debris cloud is faint at optical wavelengths. CTA 1's visible wavelength emission from still expanding shock fronts is revealed in this deep telescopic image, a frame that spans about 2 degrees across a starfield in the northern constellation of Cepheus. While no pulsar has since been found at radio wavelengths, in 2008 the Fermi Gamma-ray Space Telescope detected pulsed emission from CTA 1, identifying the supernova remnant's rotating neutron star. The source has been recognized as the first in a growing class of pulsars that are quiet at radio wavelengths but pulse in high-energy gamma-rays.

Photo by Thomas Lelu

A Simple Poem

Posted by MFish • Profile • 08/22/24 at 10:02PM • Poetry • See more by MFish

A simple poem,
it means so much,
for I may have
lost my writing touch.

A Comment by Loy

Your avatar
Loy • 08/24/2024 at 05:42PM • Like 1 • Profile

You’ve still got it!

A Comment by MFish

Your avatar
MFish • 08/24/2024 at 10:57PM • Like • Profile

Thank you. I've begun questioning my ability to writel

NASA Astronomy Picture of the Day:

In silhouette against a crowded star field along the tail of the arachnological constellation Scorpius, this dusty cosmic cloud evokes for some the image of an ominous dark tower. In fact, monstrous clumps of dust and molecular gas collapsing to form stars may well lurk within the dark nebula, a structure that spans almost 40 light-years across this gorgeous telescopic portrait. A cometary globule, the swept-back cloud is shaped by intense ultraviolet radiation from the OB association of very hot stars in NGC 6231, off the upper right corner of the scene. That energetic ultraviolet light also powers the globule's bordering reddish glow of hydrogen gas. Hot stars embedded in the dust can be seen as bluish reflection nebulae. This dark tower and associated nebulae are about 5,000 light-years away. Growing Gallery: Moon Eclipses Saturn in August 2024

Photo by Mike Selby

Of Love

Posted by MFish • Profile • 08/21/24 at 11:18PM • Poetry • See more by MFish

Of love
and loss,
of a soul,
such as she.
What happens
now, when her
soul is free.

NASA Astronomy Picture of the Day:

Forget X-ray vision — imagine what you could see with gamma-ray vision! The featured all-sky map shows what the universe looks like to NASA's Fermi Gamma-ray Space Telescope. Fermi sees light with energies about a billion times what the human eye can see, and the map combines 12 years of Fermi observations. The colors represent the brightness of the gamma-ray sources, with brighter sources appearing lighter in color. The prominent stripe across the middle is the central plane of our Milky Way galaxy. Most of the red and yellow dots scattered above and below the Milky Way’s plane are very distant galaxies, while most of those within the plane are nearby pulsars. The blue background that fills the image is the diffuse glow of gamma-rays from distant sources that are too dim to be detected individually. Some gamma-ray sources remain unidentified and topics of research — currently no one knows what they are.

"Scientific theory has had a rough time in America’s public schools...... Over the past few decades, conservative or religious groups that object to including the theory of evolution in science classes have tried a different approach. Now, they argue, if the “scientific” theory of evolution is taught, other views, such as “intelligent design” – a stand-in for creationism – should also be taught"  More at The Conversation ➜

Life is Short

Posted by MFish • Profile • 08/20/24 at 02:24PM • Poetry • See more by MFish

Life is short,
full of many treasures now.
Times change and here you are,
unable to maintain your vow.

She is gone,
away from thee.
You will never more,
her face to see.

Loneliness becomes
a part of your life,
for you no longer have,
your beautiful wife.

I miss you,
my darling soul,
but will soon be there,
and we'll be whole.

Finality

Posted by MFish • Profile • 08/20/24 at 02:24PM • Poetry • See more by MFish

The finality of life,
as we know it today,
will soon change,
and go away.

It's OK for in this,
our life's cycle here,
will bring forth a
time which we held dear.

Life must end,
this we know.
I wish to exit quietly,
as my final show.

NASA Astronomy Picture of the Day:

A supermoon occurred yesterday. And tonight's moon should also look impressive. Supermoons appear slightly larger and brighter than most full moons because they reach their full phase when slightly nearer to the Earth -- closer than 90 percent of all full moons. This supermoon was also a blue moon given the definition that it is the third of four full moons occurring during a single season. Blue moons are not usually blue, and a different definition holds that a blue moon is the second full moon that occurs during a single month. The featured image captured the blue supermoon right near its peak size yesterday as it was rising beyond the Temple of Poseidon in Greece. This supermoon is particularly unusual in that it is the first of four successive supermoons, the next three occurring in September, October, and November.

..."The latest research suggests that blood sugar fluctuations are partly responsible for the connection between what we eat and how we feel. Through its effects on our hormones and our nervous system, blood sugar levels can be fuel for anxiety and depression"... More at The Conversation ➜

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