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#vega

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You can use reactive widgets to speed up your interactive visualization application development, while also facilitating re-usability.

It is also very useful for coordinating views, even if they are written using different libraries. Here's is a simple example synchronizing #vega-lite & #d3js

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Hubble and #JWST get a very clear view of Vega.

It's a mysterious system because it's unlike other circumstellar disks. The #Vega disk is smooth, ridiculously smooth.

There is no obvious evidence for one or more large #planets plowing through the face-on #disk like snow tractors.

The Vega disk does have a subtle gap, around 60 AU from the #star, but otherwise is very smooth all the way in until it is lost in the glare of the star.

#astronomy #exoplanets
phys.org/news/2024-11-hubble-w

phys.orgHubble and Webb probe surprisingly smooth disk around VegaIn the 1997 movie "Contact," adapted from Carl Sagan's 1985 novel, the lead character scientist Ellie Arroway (played by actor Jodi Foster) takes a space-alien-built wormhole ride to the star Vega. She emerges inside a snowstorm of debris encircling the star—but no obvious planets are visible.

Today on the arXiv:

Su et al. 2024, "Imaging of the Vega Debris System using JWST/MIRI" - arxiv.org/abs/2410.23636

Wolff et al. 2024, "Deep Search for a scattered light dust halo around Vega with the Hubble Space Telescope" - arxiv.org/abs/2410.24042

Presenting complementary observations that exclude any planets larger than Neptune around #Vega , down to below 6 Earth masses for some orbits, despite the debris disc.

The authors compare to the case of #Fomalhaut .

arXiv.orgImaging of the Vega Debris System using JWST/MIRIWe present images of the Vega planetary debris disk obtained at 15.5, 23, and 25.5 microns with the Mid-Infrared Instrument (MIRI) on JWST. The debris system is remarkably symmetric and smooth, and centered accurately on the star. There is a broad Kuiper-belt-analog ring at 80 to 170 au that coincides with the planetesimal belt detected with ALMA at 1.34 mm. The interior of the broad belt is filled with warm debris that shines most efficiently at mid-infrared along with a shallow flux dip/gap at 60 au from the star. These qualitative characteristics argue against any Saturn-mass planets orbiting the star outside of about 10 au assuming the unseen planet would be embedded in the very broad planetesimal disk from a few to hundred au. We find that the distribution of dust detected interior to the broad outer belt is consistent with grains being dragged inward by the Poynting-Robertson effect. Tighter constraints can be derived for planets in specific locations, for example any planet shepherding the inner edge of the outer belt is likely to be less than 6 Earth masses. The disk surface brightness profile along with the available infrared photometry suggest a disk inner edge near 3-5 au, disconnected from the sub-au region that gives rise to the hot near-infrared excess. The gap between the hot, sub-au zone and the inner edge of the warm debris might be shepherded by a modest mass, Neptune-size planet.

#ESA:

"A redesigned Zefiro-40 solid rocket motor, the second stage of the Vega-C rocket, was successfully fired up .. at its Salto di Quirra test facility in Sardinia, Italy. This second firing follows from a first firing test of the motor in May 2024 and concludes the qualification tests for the improved engine nozzle design of the Zefiro-40."

esa.int/Enabling_Support/Space

3.10.2024

www.esa.intLast rocket motor firing clears path for Vega-C launch

🛰️ Le satellite #Sentinel2C est sous coiffe ! Il sera lancé le 4 septembre par la dernière #Vega #VV24. Il doit remplacer le satellite Sentinel-2A à une altitude de 786 km pour l'observation de la Terre et ses applications dérivées comme l'agriculture de précision, la surveillance de la qualité de l’eau et la gestion des catastrophes naturelles
📷 ESA/Airbus Space