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Deep Focus

Veriditas

Seeming

Hello. I am Aethery Fields.

There are moments when time seems to stand still.

Instants when fog settles over a landscape and contours blur. "hello." is such a moment, captured in sound, preserved like a fading Polaroid whose edges are already dissolving.
After a distant time in the shadows, sailing the cinematic seas of Dark Ambient and Soundscape with my moniker "Logic Moon", I felt the need to give my brighter side more space. **Aethery Fields** was born, not as an escape, but as a complement. A place where light penetrates through the mist, where silence is not empty but filled with fleeting impressions.

"hello." is the counterpoint to my otherwise busy self. It is a still frame in a fog-veiled landscape, blurred, hazy, yet all the more haunting for it. Sometimes they are mere silhouettes drifting through the sound, vague intimations of melodies that emerge from the mist and vanish again. Then suddenly simple lines crystallize, clear and immediate, before fading back into the haze.

Process
Every track on this album emerged spontaneously, born from the moment itself. I sat down, pressed record, and let the things flow. No overthinking, no perfectionism, only the urge to capture the here and now before it slips away. What you hear is what happened in that instant. A texture, a melody appearing out of nowhere. Minimalist in form, yet rich in emotion. This music reveals my quiet side, that self which strives for deceleration, which dwells in the now and transforms impressions into sound as naturally as breathing. Each piece is an impulse made audible, a fleeting thought given form. It is a pause between breaths, a lingering in the moment before it dissolves.

Like a Polaroid capturing the essence of a vanishing moment, the diffuse light, the blurred atmosphere, the unrepeatable accident, "hello." reflects instants that can never be fully grasped or recreated. Still lifes in stillness, which despite their calm are permeated by countless sounds and impressions. It is the beauty of the imperfect, the transient, the barely visible, the unplanned.
"hello." is an invitation to pause, to lose yourself in the fog and to discover the essential in the blurred, to feel the aliveness within the stillness.

hello.

Song1

151 - Softened Light

Into the Beyond

HOLI Byte
Stellar Evolution - The life story of stars
Hands On Learning Initiative
Content: Gayathri Raman
Voice: Gayathri Raman
Introduction: Priyanka Singh
Editing: Mayuri Rao

SHOW NOTES:
Stars are like fiery hot balls of gas, held together as one massive globule with the help of gravity. Like humans, they are born, have a finite life time during which they age, and finally die. The initial mass with which a particular star is born, decides how it evolves.  Take for example a star like the sun, whose mass is roughly 2 times 10 to the power 30 kg, that is, 2 followed by 30 zeros. It fuses hydrogen to helium for a few billion years.  During this period,  gravity tries pulling all the matter inwards while radiation, from burning hydrogen, exerts pressure outwards, that is in a direction opposite to that of gravity. The burning of Hydrogen keeps the tug-of-war between gravity and radiation going. As the amount of hydrogen starts decreasing, the star grows into a massive red giant. As the name suggests the star has a reddish colour and grows in size because of the thin layer of Hygrogen that surrounds a small helium core. In fact, when our sun becomes a red giant, it will grow so big in size that it will engulf all the inner planets of the Solar system, including the earth. After all the hydrogen fuel gets exhausted, gravity starts over-powering the outward radiation pressure, making the ball of gas collapse on itself. This is when things start getting exciting and stellar fates diverge.  For sun-sized stars, the core starts collapsing while the outer shell starts expanding and is eventually blown away leaving behind a white dwarf star, that is hot, less luminous and nearly the size of the earth. For stars, born with roughly twice the mass of our Sun, the cores collapse further. They undergo a massive expsion called a supernova and end up as neutron stars, that are roughly the size of a small city with a 10 km radius. A different kind of pressure, called the Fermi degeneracy pressure, exerted by fermions that are particles like electrons and neutrons, prevent White Dwarfs and Neutron stars from collapsing further. But what if there is a star that is really really massive? Such stars, with masses many times the mass of our sun, explode brilliantly and finally form a black hole. No kind of pressure can counter gravity in black holes. Even light, or more generally, electromagnetic radiation, cannot escape from these notorious objects. 
When you look up at the night sky and see the countless number of stars, remember each star has its own story!

References:


HOLI byte

HOLI Byte: Stellar Evolution - English

Stellar Evolution - The life story of stars

Glaciers, taken from the new mini-album Bloom. 
Out everywhere where music lives. 

www.lightsandmotion.com

Bloom

Glaciers

Cooper Sams - Adrift

"Moiety" is a new Helios album free for download at http://www.unseen-music.com/free .

Dreams Of Another Reality

August Wilhelmsson

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