By @_nastya_

By @_nastya_
By @_nastya_
By @_nastya_

By @_nastya_

More Posts from Aideeramirez and Others

3 years ago
Ukyomi
Ukyomi
Ukyomi

ukyomi

3 years ago
SWEET TOOTH Yields One Cocktail

SWEET TOOTH Yields one cocktail

2 1⁄2 oz vodka 1⁄2 oz St. Germain Champagne float Raw sugar rim

Instructions: Add vodka and St. Germain into a cocktail shaker with ice, shake well and strain into a sugar-rimmed glass. Top with a champagne float.

2 years ago
I Do Believe Marsellus My Husband,your Boss, Told You To Take Me Out And Do Whatever ı Wanted. Now ı

I do believe Marsellus my husband,your boss, told you to take me out and do whatever ı wanted. Now ı wanna dance, ı wanna win. I want that trophy, so dance good.

1 year ago
Cindy Reis By Alberto Pelayo For Numéro Netherlands July 2023
Cindy Reis By Alberto Pelayo For Numéro Netherlands July 2023
Cindy Reis By Alberto Pelayo For Numéro Netherlands July 2023
Cindy Reis By Alberto Pelayo For Numéro Netherlands July 2023

Cindy Reis by Alberto Pelayo for Numéro Netherlands July 2023

2 years ago

solar system size comparison

Via astrolover

3 years ago
Blanet: A New Class Of Planet That Could Form Around Black Holes
Blanet: A New Class Of Planet That Could Form Around Black Holes
Blanet: A New Class Of Planet That Could Form Around Black Holes

Blanet: A new class of planet that could form around black holes

The dust clouds around supermassive black holes are the perfect breeding ground for an exotic new type of planet.

Blanets are fundamentally similar to planets; they have enough mass to be rounded by their own gravity, but are not massive enough to start thermonuclear fusion, just like planets that orbit stars. In 2019, a team of astronomers and exoplanetologists showed that there is a safe zone around a supermassive black hole that could harbor thousands of blanets in orbit around it.

The generally agreed theory of planet formation is that it occurs in the protoplanetary disk of gas and dust around young stars. When dust particles collide, they stick together to form larger clumps that sweep up more dust as they orbit the star. Eventually, these clumps grow large enough to become planets.

A similar process should occur around supermassive black holes. These are surrounded by huge clouds of dust and gas that bear some similarities to the protoplanetary disks around young stars. As the cloud orbits the black hole, dust particles should collide and stick together forming larger clumps that eventually become blanets.

The scale of this process is vast compared to conventional planet formation. Supermassive black holes are huge, at least a hundred thousand times the mass of our Sun. But ice particles can only form where it is cool enough for volatile compounds to condense.

This turns out to be around 100 trillion kilometers from the black hole itself, in an orbit that takes about a million years to complete. Birthdays on blanets would be few and far between!

An important limitation is the relative velocity of the dust particles in the cloud. Slow moving particles can collide and stick together, but fast-moving ones would constantly break apart in high-speed collisions. Wada and co calculated that this critical velocity must be less than about 80 meters per second.

source

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aideeramirez - D For Style
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