HW: 101.6kg | LW: 54 | CW: 89 | GW1: 85 | GW2: 75 | GW3: 65 | GW4: 55 | UGW: 45
23 posts
me, eating a fear food:
ana:
hi i need mutuals + people to support and get support from bc im scared im gonna give up and be really fucking fat
reblog if ur
-16 + or -
-not pro anything
-just starting or can support
-active as of dec. 2019
-post thinspo or updates or diets!!!
-bruh literally anything i need mutuals on here :((((
ok bye
Reblog if you’re in the Yes-I-Have-An-Eating-Disorder-No-You-Shouldn’t-Starve-Yourself club
You did this. You drove me back to these bad habits. This ED is resurfaced because of you.
my followers watching me reblog yet another "weight loss fairy" knowing full well i wont lose any weight:
Tumblr after terminating our blogs:
bitches be telling herself everey week shes gonna start now but then eating like shit everyday and ditching the gym everytime and doesnt workout & wonders why shes gaining weight.
its me. Im bitches
Losing weight but only in my boobs and butt
I lose weight and don’t gain it back
It this ain't an illness, I don't know what it is.
hey siri, delete my fat
As the Spitzer Space Telescope’s 16-year mission ends, we’re celebrating the legacy of our infrared explorer. It was one of four Great Observatories – powerful telescopes also including Hubble, Chandra and Compton – designed to observe the cosmos in different parts of the electromagnetic spectrum.
The part of the spectrum we can see is called, predictably, visible light. But that’s just a small segment of all the wavelengths of the spectrum. The Hubble Space Telescope observes primarily in the visible spectrum. Our Chandra X-ray Observatory is designed to detect (you guessed it) X-ray emissions from very hot regions of the universe, like exploded stars and matter around black holes. Our Compton Gamma Ray Observatory, retired in 2000, produced the first all-sky survey in gamma rays, the most energetic and penetrating form of light.
Infrared radiation, or infrared light, is another type of energy that we can’t see but can feel as heat. All objects in the universe emit some level of infrared radiation, whether they’re hot or cold. Spitzer used its infrared instrument to make discoveries in our solar system (including Saturn’s largest ring) all the way to the edge of the universe. From stars being born to planets beyond our solar system (like the seven Earth-size exoplanets around the star TRAPPIST-1), Spitzer’s science discoveries will continue to inspire the world for years to come.
Together, the work of the Great Observatories gave us a more complete view and understanding of our universe.
Hubble and Chandra will continue exploring our universe, and next year they’ll be joined by an even more powerful observatory … the James Webb Space Telescope!
Many of Spitzer’s breakthroughs will be studied more precisely with the Webb Space Telescope. Like Spitzer, Webb is specialized for infrared light. But with its giant gold-coated beryllium mirror and nine new technologies, Webb is about 1,000 times more powerful. The forthcoming telescope will be able to push Spitzer’s science findings to new frontiers, from identifying chemicals in exoplanet atmospheres to locating some of the first galaxies to form after the Big Bang.
We can’t wait for another explorer to join our space telescope superteam!
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Me eating, ever:
He is my spirit animal 🙌🏻🙌🏻🙌🏻
the dream team