
Una nueva imagen de alta definición de la NASA's James Webb Space Telescope (cámara de infrarrojo cercano) revela detalles intrincados de la supernova remanente de cassiopeia a (Cas a), y muestra la carcasa expansiva de los golpes de material en la estrella de la estrella de la estrella de la estrella y los colores más livianos de los colores más livianos de la red de los colores más livianos de la imagen de los colores más livianos de la cebada de los accesorios. Concha interior del remanente de supernova. Estos pequeños nudos de gas, compuestos por azufre, oxígeno, argón y neón de la estrella misma, solo son detectables por la resolución exquisita de Nircam, y brindan a los investigadores una pista de cómo la estrella moribunda se rompió como el vidrio cuando explota. Esto marca donde el material expulsado de la estrella explotada se está embarcando en el material circunstelar circundante. Los investigadores dicen que este color blanco es ligero de la radiación sincrotrón, que se genera por partículas cargadas que viajan a velocidades extremadamente altas en espiral alrededor de las líneas de campo magnético.
También hay varios ecos de luz visibles en esta imagen, especialmente en la esquina inferior derecha. Aquí es donde ha alcanzado la luz de la explosión de la estrella, y está calentando el polvo distante, que está brillando a medida que se enfría.
créditos
Image
NASA, ESA, CSA, STSCI, Danny Milisavljevic (Universidad Purdue), ilse de LOOZE (UGENT), TEAT), TEAT), TEAT). Universidad)
About The Object | |
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Object Name | Cassiopeia A; SNR G111.7-02.1 |
Object Description | Supernova remnant |
R.A. Position | 23:23:24.00 |
Dec. Position | +58:48:54.00 |
Constellation | Cassiopeia |
Distance | 11,090 light-years |
Dimensions | Image is about 5.8 arcminutes across (19 light-years). |
About The Data | |
Data Description | This image was created with Webb data from proposal: (D. Milisavljevic). |
Instrument | NIRCam |
Exposure Dates | 05 November 2022 |
Filters | F162M, F356W, F444W |
About The Image | |
Color Info | These images are a composite of separate exposures acquired by the James Webb Space Telescope using the NIRCam instrument. Several filters were used to sample specific wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F162M, Green: F356W, Red: F444W |
Compass Image | ![]() |
About The Object | |
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Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
Object Description | The type of astronomical object. |
R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
Distance | The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs. |
Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
About The Data | |
Data Description |
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Instrument | The science instrument used to produce the data. |
Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
Filters | The camera filters that were used in the science observations. |
About The Image | |
Image Credit | The primary individuals and institutions responsible for the content. |
Publication Date | The date and time the release content became public. |
Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |