emely-renderos

[emely-renderos]

Aún tengo cartas que no me atrevo a enviarte.

[emely-renderos]

Te mereces el mundo entero, todo el mundo puede ver lo increíble que eres menos tú.

Misteriosa como el mar.

[emely-renderos]

A veces conoces a una persona y se produce automáticamente un clic; te sientes a gusto con ella, como si la hubieras conocido toda tu vida y no tuvieras que fingir ni hacerte pasar por lo que no eres.

[emely-renderos]

Cómo te digo que te quiero si sé que no sientes lo mismo.

~Alessa

[emely-renderos]

“Y de mucho sufrir o tanto vivir, te das cuenta que el guion de la vida siempre incluye pasajes de dolor, etapas derroteras, esperanzas redentoras o ilusiones de “todo pasado fue mejor”, momentos dichosos de “todo está conectado”. Todo ello es sabiduría de tu viaje sin retorno. Vive sin aferrarte a lo efímero como eterno, hay más crónicas no escritas esperándote.”

— Firthunands

[emely-renderos]

[emely-renderos]

Aunque se hable mil lenguas, nos cuesta pedir ayuda, consuelo, compañía, cariño.

Firthunands (via oceano-de-letras)

[emely-renderos]

Decoding Nebulae

We can agree that nebulae are some of the most majestic-looking objects in the universe. But what are they exactly? Nebulae are giant clouds of gas and dust in space. They’re commonly associated with two parts of the life cycle of stars: First, they can be nurseries forming new baby stars. Second, expanding clouds of gas and dust can mark where stars have died.

Not all nebulae are alike, and their different appearances tell us what's happening around them. Since not all nebulae emit light of their own, there are different ways that the clouds of gas and dust reveal themselves. Some nebulae scatter the light of stars hiding in or near them. These are called reflection nebulae and are a bit like seeing a street lamp illuminate the fog around it.

In another type, called emission nebulae, stars heat up the clouds of gas, whose chemicals respond by glowing in different colors. Think of it like a neon sign hanging in a shop window!

Finally there are nebulae with dust so thick that we’re unable to see the visible light from young stars shine through it. These are called dark nebulae.

Our missions help us see nebulae and identify the different elements that oftentimes light them up.

The Hubble Space Telescope is able to observe the cosmos in multiple wavelengths of light, ranging from ultraviolet, visible, and near-infrared. Hubble peered at the iconic Eagle Nebula in visible and infrared light, revealing these grand spires of dust and countless stars within and around them.

The Chandra X-ray Observatory studies the universe in X-ray light! The spacecraft is helping scientists see features within nebulae that might otherwise be hidden by gas and dust when viewed in longer wavelengths like visible and infrared light. In the Crab Nebula, Chandra sees high-energy X-rays from a pulsar (a type of rapidly spinning neutron star, which is the crushed, city-sized core of a star that exploded as a supernova).

The James Webb Space Telescope will primarily observe the infrared universe. With Webb, scientists will peer deep into clouds of dust and gas to study how stars and planetary systems form.

The Spitzer Space Telescope studied the cosmos for over 16 years before retiring in 2020. With the help of its detectors, Spitzer revealed unknown materials hiding in nebulae — like oddly-shaped molecules and soot-like materials, which were found in the California Nebula.

Studying nebulae helps scientists understand the life cycle of stars. Did you know our Sun got its start in a stellar nursery? Over 4.5 billion years ago, some gas and dust in a nebula clumped together due to gravity, and a baby Sun was born. The process to form a baby star itself can take a million years or more!

After billions more years, our Sun will eventually puff into a huge red giant star before leaving behind a beautiful planetary nebula (so-called because astronomers looking through early telescopes thought they resembled planets), along with a small, dense object called a white dwarf that will cool down very slowly. In fact, we don’t think the universe is old enough yet for any white dwarfs to have cooled down completely.

Since the Sun will live so much longer than us, scientists can't observe its whole life cycle directly ... but they can study tons of other stars and nebulae at different phases of their lives and draw conclusions about where our Sun came from and where it's headed. While studying nebulae, we’re seeing the past, present, and future of our Sun and trillions of others like it in the cosmos.

To keep up with the most recent cosmic news, follow NASA Universe on Twitter and Facebook.

Make sure to follow us on Tumblr for your regular dose of space.

[emely-renderos]

Hay personas que llegan y nos revolucionan de tal manera que nos convierten en alguien más.

Alaska

[emely-renderos]

Beetlejuice (1988)

[emely-renderos]

mi dispiace essere così, davvero. perdonami

[emely-renderos]

Estoy más tranquilo sabiendo que ya no hay vuelta atrás.

Blazze

[emely-renderos]

Elvis Presley - Can’t Help Falling In Love 

[emely-renderos]

Lunes 16 de Enero: Llegaste como un bello atardecer sin ser esperado, apareciendo de la nada deslumbrandome con tu divinidad logrando captar mi atención  tanto que regresaba todos los días para seguir contemplando tan majestuosa vista y desde ese día supe que quería admirar ese atardecer por el resto de mi vida Yo creo que en esta vida para cada persona existe su atardecer destinado, ese atardecer que te deslumbra tanto que te hace querer verlo por toda la eternidad.

Poesía original de @imyluu (via poesia-en-la-lengua)

[emely-renderos]

Para aquellos, que como yo, crecieron viendo un clásico.

Floricienta / Flores Amarillas

[emely-renderos]

Nunca pensé tener una playlist especial para vos y menos espere incluir floricienta ahí.

[emely-renderos]

No quiero más promesas de amor, quiero que hagamos las cosas sin pensar. Quiero arriesgarme más, por ti.

Cam.