The fourth team, coached by Terry, will be composed of the aforementioned G League representatives. Gasol, Noah and Williams drafted their seven-player teams on Feb. Location: Vivint Arena - Salt Lake City, Utahįormer NBA All-Stars Pau Gasol, Joakim Noah and Deron Williams will serve as coaches for the three NBA Rising-Star teams, while former Sixth Man of the Year Jason Terry will lead the G League team. The teams will participate in a mini-tournament featuring the always-exciting Elam Ending with a final target score.īelow you'll find viewing information and the format for the event, along with the full rosters. The format has shifted over the years in order to make the game more competitive - it had a tendency to devolve into an impromptu dunk contest in the fourth quarter - and this time around there will be four teams coached by prominent ex- NBA players. The league's fresh crop young talent will be on display during All-Star Weekend in Salt Lake City, starting with the Jordan Rising Stars game on Friday night. In their early 20s (and sometimes teens), players like Luka Doncic, Zion Williamson, Trae Young, Anthony Edwards, Tyrese Haliburton and Ja Morant have already become All-Stars and, in some cases, the leaders of championship contenders. In particular, by plotting a HR diagram for either a globular or open cluster of stars, astronomers can estimate the age of the cluster from where stars appear to turnoff the main sequence (see the entry on main sequence for how this works).Over the last few seasons, young NBA talent has seemingly improved at astronomical rates. The Sun is found on the main sequence with a luminosity of 1 and a temperature of around 5,400 Kelvin.Īstronomers generally use the HR diagram to either summarise the evolution of stars, or to investigate the properties of a collection of stars. These stars are very hot but have low luminosities due to their small size. white dwarf stars (luminosity class D) are the final evolutionary stage of low to intermediate mass stars, and are found in the bottom left of the HR diagram.Stars enter this evolutionary stage once they have exhausted the hydrogen fuel in their cores and have started to burn helium and other heavier elements. They have low surface temperatures and high luminosities which, according to the Stefan-Boltzmann law, means they also have large radii. red giant and supergiant stars (luminosity classes I through III) occupy the region above the main sequence.Main sequence stars have a Morgan-Keenan luminosity class labelled V. It is here that stars spend about 90% of their lives burning hydrogen into helium in their cores. The main sequence stretching from the upper left (hot, luminous stars) to the bottom right (cool, faint stars) dominates the HR diagram. There are 3 main regions (or evolutionary stages) of the HR diagram: Also plotted are the Morgan-Keenan luminosity classes that distinguish between stars of the same temperature but different luminosity. The giant branch is also well populated and there are many white dwarfs. By far the most prominent feature is the main sequence, which runs from the upper left (hot, luminous stars) to the bottom right (cool, faint stars) of the diagram. This Hertzsprung-Russell diagram shows a group of stars in various stages of their evolution. The giant branch and supergiant stars lie above the main sequence, and white dwarfs are found below it. By far the most prominent feature is the main sequence (grey), which runs from the upper left (hot, luminous stars) to the bottom right (cool, faint stars) of the diagram. The Hertzsprung-Russell diagram the various stages of stellar evolution.
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