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Horizontal axis: Comoving distance in billion light years. Vertical axes: time since Big Bang in billions of years Shown are the Particle Horizon RP (green), Event Horizon RE (magenta), Hubble Radius RH (blue). Past and future light cones RL (orange) are animated. Dashed grey lines are lines of constant comoving distances (i.e. the Hubble flow).
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Animation_of_Parker_Solar_Probe_trajectory.webm (WebM audio/video file, VP9, length 1 min 27 s, 560 × 420 pixels, 156 kbps overall, file size: 1.61 MB) This is a file from the Wikimedia Commons . Information from its description page there is shown below.
Animations can be generated ad hoc in a browser with the CSS 3 features animations, transitions, and sprites, or also the JavaScript web animations API, by specifying frames or motions of still images or rendered shapes. This can be resource-intensive, and the animation generally cannot be saved in a portable image file or posted on imageboards.
English: James Webb Space Telescope orbit as seen from above the Sun's north pole and as seen from Earth's perspective. The James Webb Space Telescope will not be in orbit around the Earth, like the Hubble Space Telescope is - it will actually orbit the Sun, 1.5 million kilometers (1 million miles) away from the Earth at what is called the second Lagrange point or L2.
Original file (WebM audio/video file, VP9, length 5 min 7 s, 1,920 × 1,080 pixels, 5.16 Mbps overall, file size: 188.47 MB) This is a file from the Wikimedia Commons . Information from its description page there is shown below.
In 2015, Anime Studio 11 added frame-by-frame animation, layer referencing, animated shape ordering, enhanced tools and brushes, JSON file format support, and other features. In 2016, Anime Studio was rebranded as its original name Moho by Smith Micro Software to reflect the software's ability to create more animated content than anime.
English: Movie of the solar photosphere observed with the Swedish 1-m Solar Telescope (SST) on La Palma, Spain. The movie shows solar granulation which is a result of convective motions of bubbles of hot gas that rise from the solar interior.