I wear it for the pollution almost everyone around me is putting into the air I need to breath.
Plot twist: two other bears are also humans in bear suites.
I appreciate you. I cycle almost everyday, and the amount of times I've been put into dangerous situations because of someone else's impatience is way too high.
I've been through a similar process (as an employee) and all I can keep thinking is "Fuck you." after every sentence this guy says.
Yes.
Allow me to interject for a moment
REEEEEEEEEEEEEEEEEE
GIRAFFE GIRAFFE GIRAFFE GIRAFFE GIRAFFE GIRAFFE GIRAFFE GIRAFFE GIRAFFE GIRAFFE GIRAFFE GIRAFFE GIRAFFE
I usually play it in short bursts, iirc you can save at any time.
*flipper slapping intensifies
[Image description: The two galaxies swirl into a single chaotic object in the centre. Long, blue spiral arms stretch vertically, faint at the edges. Hot gas spreads horizontally over that, mainly bright red with many small gold spots of star formation. The core of the merging galaxies is very bright and radiates eight large, golden diffraction spikes. The background is black, with many tiny galaxies in orange and blue.]
[Image Description: A close-up view of a barred spiral galaxy. Two spiral arms reach horizontally away from the core in the centre, merging into a broad network of gas and dust which fills the image. This material glows brightest orange along the path of the arms, and is darker red across the rest of the galaxy. Through many gaps in the dust, countless tiny stars can be seen, most densely around the core.]
[Image Description: A large spiral galaxy takes up the entirety of the image. The core is mostly bright white, but there are also swirling, detailed structures that resemble water circling a drain. There is white and pale blue light that emanates from stars and dust at the core’s centre, but it is tightly limited to the core. The rings feature colours of deep red and orange and highlight filaments of dust around cavernous black bubbles.]
[Image description: A close-in image of a spiral galaxy, showing its core and part of a spiral arm. Thousands upon thousands of tiny stars that make it up can be seen, most dense in a whitish bar that forms its core. Clumps and filaments of dust form an almost skeletal structure that follows the twist of the galaxy and its spiral arm. Large, glowing bubbles of red gas are hidden in the dust.]
[Image Description: A huge, dense field completely filled with tiny stars. A few of the star images are a bit larger than the rest, with visible diffraction spikes; two foreground stars are large and bright on the right side. Many small galaxies within various shapes and sizes can be seen hiding behind the stars. In the centre some faint, wispy, dark red gas appears.] or [Image Description: A huge, dense field completely filled with stars. A few of the star images are a bit larger than the rest, with visible diffraction spikes; two foreground stars are bright on the right side. Many galaxies with various shapes and sizes can be seen hiding behind the stars. In the centre some faint, wispy, dark red gas appears.]
https://esawebb.org/images/weic2212a/
[Image Description: [Shoe horned] In this mosaic image stretching 340 light-years across, Webb’s Near-Infrared Camera (NIRCam) displays the Tarantula Nebula star-forming region in a new light, including tens of thousands of never-before-seen young stars that were previously shrouded in cosmic dust. The most active region appears to sparkle with massive young stars, appearing pale blue. Scattered among them are still-embedded stars, appearing red, yet to emerge from the dusty cocoon of the nebula. NIRCam is able to detect these dust-enshrouded stars thanks to its unprecedented resolution at near-infrared wavelengths.
To the upper left of the cluster of young stars, and the top of the nebula’s cavity, an older star prominently displays NIRCam’s distinctive eight diffraction spikes, an artefact of the telescope’s structure. Following the top central spike of this star upward, it almost points to a distinctive bubble in the cloud. Young stars still surrounded by dusty material are blowing this bubble, beginning to carve out their own cavity. Astronomers used two of Webb’s spectrographs to take a closer look at this region and determine the chemical makeup of the star and its surrounding gas. This spectral information will tell astronomers about the age of the nebula and how many generations of star birth it has seen.
Farther from the core region of hot young stars, cooler gas takes on a rust colour, telling astronomers that the nebula is rich with complex hydrocarbons. This dense gas is the material that will form future stars. As winds from the massive stars sweep away gas and dust, some of it will pile up and, with gravity’s help, form new stars.]
Anthophila