Birth Of a New Star Captured By James Webb

[{"selector":"#anim-4c53db4d-5f7d-4484-b452-2c1bdaee17b7","keyframes":{"opacity":[0,1]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-5a539b5a-51d6-4eee-9585-f463f6143c5e","keyframes":{"transform":["translate3d(0px, 143.02422%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-83a44257-3978-4ae5-a55e-de3219c33be9 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(-61.268952185145444%, 0, 0) translate(-25%, 0%) scale(1.5)","translate3d(0%, 0, 0) translate(0%, 0%) scale(1)"]},"delay":0,"duration":2000,"fill":"forwards"}] A new image of a Herbig-Haro object captured by the James Webb Space Telescope shows the dramatic outflows from a young star.

[{"selector":"#anim-9755c9fe-aff5-497a-8801-198ece43ad55","keyframes":{"opacity":[0,1]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-9841a349-e596-4355-a868-b2c5ec688b8b","keyframes":{"transform":["translate3d(0px, 201.52785%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-422bb2e7-042b-47b5-bb09-6220ba180ee4 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(60.4880704881104%, 0, 0)","translate3d(0%, 0, 0)"]},"delay":0,"duration":2000,"easing":"cubic-bezier(.3,0,.55,1)","fill":"both"}] These luminous flares are created when stellar winds shoot off in opposite directions from newborn stars

[{"selector":"#anim-93374989-0be1-4311-adcd-bfb857657080","keyframes":{"opacity":[0,1]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-2aff623c-740b-4dd8-8a96-31c9deeef045","keyframes":{"transform":["translate3d(0px, 168.01935%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-3d076f42-8d71-43ec-bfb2-3c2289f74194 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(-40.25127720131342%, 0, 0) translate(-25%, 0%) scale(1.5)","translate3d(0%, 0, 0) translate(0%, 0%) scale(1)"]},"delay":0,"duration":2000,"fill":"forwards"}] These objects can be huge, up to several light-years across, and they glow brightly in the infrared wavelengths in which James Webb operates.

[{"selector":"#anim-f8b0f7f1-4a84-4fc4-8fe5-ab3f91ed74d5","keyframes":{"opacity":[0,1]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-455329da-ddda-4c0f-b269-f9f992565779","keyframes":{"transform":["translate3d(0px, 173.42504%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-d57cc691-cf99-41d0-b998-b8136a8538e1 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(-38.03335324622852%, 0, 0) translate(-25%, 0%) scale(1.5)","translate3d(0%, 0, 0) translate(0%, 0%) scale(1)"]},"delay":0,"duration":2000,"fill":"forwards"}] This image shows Herbig-Haro object HH 797, which is located close to the IC 348 star cluster,

[{"selector":"#anim-925490d4-6513-4df7-8fc5-6494d8806f10","keyframes":{"opacity":[0,1]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-6b2f2487-946d-431d-be35-b1e48bd64213","keyframes":{"transform":["translate3d(0px, 219.02784%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-46ed1486-cf84-494a-9081-6bb067661258 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(-35.299816060549325%, 0, 0) translate(-25%, 0%) scale(1.5)","translate3d(0%, 0, 0) translate(0%, 0%) scale(1)"]},"delay":0,"duration":2000,"fill":"forwards"}] The image was taken using Webb’s Near-Infrared Camera (NIRCam) instrument,

[{"selector":"#anim-b7990e0d-ed06-4812-82d3-de094b6efbf1","keyframes":{"opacity":[0,1]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-b5ae1b80-bd1f-4153-bebe-f6ddff0dc768","keyframes":{"transform":["translate3d(0px, 180.64150%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-65ac18cf-7d5d-4a15-af98-451871032bf5 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(30.258452943555376%, 0, 0)","translate3d(0%, 0, 0)"]},"delay":0,"duration":2000,"easing":"cubic-bezier(.3,0,.55,1)","fill":"both"}] Webb scientists explain in a statement, : “Infrared imaging is a powerful way to study newborn stars and their outflows

[{"selector":"#anim-decc9b90-068f-4bf2-955f-4d04ea5e09d0","keyframes":{"opacity":[0,1]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-8f86a4a8-cd39-459a-bf4f-0435c16935c2","keyframes":{"transform":["translate3d(0px, 178.57967%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-7ebb7440-faae-42c0-859f-176b3095a7b7 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(-42.58477678445608%, 0, 0) translate(11.832061068702288%, 11.832060605499153%) scale(0.7633587786259542)","translate3d(0%, 0, 0) translate(0%, 0%) scale(1)"]},"delay":0,"duration":2000,"fill":"forwards"}] This particular Herbig-Haro object is unusual in that scientists originally believed that it was created from a single young star, as most such objects are.

[{"selector":"#anim-1d8c04b1-eeca-4893-aa20-9bd91599365a","keyframes":{"opacity":[0,1]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-c36cf995-3b34-4e5a-8296-da37aa117fe3","keyframes":{"transform":["translate3d(0px, 181.67241%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-b44f76d3-713d-4bec-931f-14b9f4048ac5 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(-15.540768282745068%, 0, 0) translate(-25%, 0%) scale(1.5)","translate3d(0%, 0, 0) translate(0%, 0%) scale(1)"]},"delay":0,"duration":2000,"fill":"forwards"}] But these detailed observations reveal that there are actually two sets of outflows, coming from a pair of stars at the center.

[{"selector":"#anim-90699386-9882-41e2-bae7-ab5abe3347a7","keyframes":{"opacity":[0,1]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-2f18c915-bbdb-4fb6-9b6a-7f8106ae519c","keyframes":{"transform":["translate3d(0px, 189.02787%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":600,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-eba7877d-d544-44c0-8c35-a18b3f6e641b [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(45.44034131446579%, 0, 0) translate(25%, 0%) scale(1.5)","translate3d(0%, 0, 0) translate(0%, 0%) scale(1)"]},"delay":0,"duration":2000,"fill":"forwards"}] The bright smudge in shades of yellow and green is believed to host two young protostars.