
Carbon Dioxide Greenhouse Effect1970-01-01T00:00:00+00:00CARBON DIOXIDE CO2 & THE GREENHOUSE EFFECT: a photon (shown as a whitish elongated ovoid) from the sun strikes the land. The land warms and emits an infrared photon (shown as a pink elongated ovoid). This IR photon strikes the carbon dioxide molecule a...PT20Shttps://d38zjy0x98992m.cloudfront.net/97456a74-dfdf-4d9b-93cd-e09d620feebb/CO2_Greenhouse_Random_HD_265_xlarge.jpghttps://d38zjy0x98992m.cloudfront.net/97456a74-dfdf-4d9b-93cd-e09d620feebb/CO2_Greenhouse_Random_HD_265_mp4_hd_video.mp4https://www.scientific.pictures/-/galleries/physics/-/medias/97456a74-dfdf-4d9b-93cd-e09d620feebb/pricehttps://www.scientific.pictures/-/galleries/physics/-/medias/97456a74-dfdf-4d9b-93cd-e09d620feebb/price
Black Hole with an orbiting body describing a rosette
Black Hole with an orbiting body describing a rosette. The simulation begins with a body (or satellite, shown as a yellow ball) with a certain velocity that is tangential to a Black Hole (shown as a bluish body in the centre). The resulting orbit creates a flower-like pattern or rosette. Notice how the object speeds up as it approaches the singularity. This is shown by the tracer balls being more widely spaced. Once the movie has fully appeared you can move the slider back and forth to see these effects at different speeds. Rosette or rose shaped orbits occur when a body (red sphere) orbits around an attractor (yellow sphere) and the force pulling the body to the attractor is inversely proportional to its distance from the attractor (proportional to 1/r). Because the force gets stronger the closer the body gets, it speeds up as it approaches the attractor (the pink tracer dots are further apart near the attractor).
Animation ID: Black-Hole-Rosetta-FHD-Russell-Kightley
Duration: 0:49
copyright Russell Kightley
Animation resolution: 1920x1080 pixels @ 30.0 fps, ~5.3 Mbits/s
Animation keywords: 1/r, astronomy, astrophysics, attracted, attractor, black, black hole, cosmology, flower, force, hole, inverse, inversely, inversely proportional to r, mathematics, orbit, orbital, physics, point attractor, proportional, rose, rosette, satellite, space, stars, tangential, universe, velocity
Black Hole with an orbiting body describing a rosette2020-08-17T08:09:57ZBlack Hole with an orbiting body describing a rosette. The simulation begins with a body (or satellite, shown as a yellow ball) with a certain velocity that is tangential to a Black Hole (shown as a bluish body in the centre). The resulting orbit creat...PT49Shttps://d3e1m60ptf1oym.cloudfront.net/8ec402c5-a38f-4885-af2e-682f1cba418e/Black-Hole-Rosetta-FHD-Russell-Kightley_xlarge.jpghttps://d3e1m60ptf1oym.cloudfront.net/8ec402c5-a38f-4885-af2e-682f1cba418e/Black-Hole-Rosetta-FHD-Russell-Kightley_mp4_hd_video.mp4https://www.scientific.pictures/-/galleries/physics/-/medias/8ec402c5-a38f-4885-af2e-682f1cba418e/pricehttps://www.scientific.pictures/-/galleries/physics/-/medias/8ec402c5-a38f-4885-af2e-682f1cba418e/price

https://d38zjy0x98992m.cloudfront.net/81888aa3-f7df-4c7b-8d0c-a7a1e49d8b08/Supercavitation_approaching_side_view_xlarge.jpghttps://www.scientific.pictures/-/galleries/physics/-/medias/81888aa3-f7df-4c7b-8d0c-a7a1e49d8b08/pricehttps://www.scientific.pictures/-/galleries/physics/-/medias/81888aa3-f7df-4c7b-8d0c-a7a1e49d8b08/price