Could S5-HVS1keep its planets?

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In summary, astronomers have detected an ultrafast star, known as S5-HVS1, traveling at 6 million km/h. It was ejected from the supermassive black hole at the center of the Milky Way five million years ago. There is speculation on whether this star had planets during its journey and if they would have been able to survive the ejection. Some experts believe that the planets may have diverged from their original trajectory due to the extreme results of this event. However, others argue that the acceleration of the star is not significantly different from other stars in the galaxy and it would not have a major effect on the planets' orbits.
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DavidCummings
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If S5-HVS1 ever had planets, would they all get stripped off when the star was ejected from the galaxy?
"Astronomers have spotted an ultrafast star [S5-HVS1], traveling at a blistering 6 million km/h, that was ejected by the supermassive black hole at the heart at the Milky Way five million years ago." -- https://www.sciencedaily.com/releases/2019/11/191112110238.htm

If this star had planets 5 million years ago, when it began its "blistering" journey, could it have held on to any of those planets, or would they all have been stripped off at the time of ejection?

Thanks.
 
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Gravitational slingshots produce fairly precise trajectories based on the gravity of the body doing the slingshotting and the closeness of the passby. NASA has made very precise use of this fact. Given the rather extreme results of this apparent event, I would think it likely that the planets would have had enough of a different distance to result is a slightly different trajectory that would likely have caused them to diverge, subsequently, from their sun.
 
  • #3
I disagree with phinds. It's going fast, but not crazy fast: about 7x faster than the sun. The star making the closest approach to Sag A* is called S2, traveling 3x faster than that. Just ballparking it, that means a closest approach of around 7 light days and an acceleration of 1.5 x 10-2 m/s2. An earth-like orbit is at 8 light minutes, so the differential acceleration is ~10-5 m/s2. This is much smaller than the actual acceleration of 6 x 10-3 m/s2.

You're probably OK up to the orbit of Saturn or so.


 
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Likes Dragrath and phinds

1. Could S5-HVS1 potentially keep its planets in orbit?

It is possible that S5-HVS1 could keep its planets in orbit, but it would depend on a variety of factors such as the mass and distance of the planets from the star, as well as the strength of the star's gravitational pull.

2. How does the high velocity of S5-HVS1 affect its ability to keep planets?

The high velocity of S5-HVS1 could potentially disrupt the orbits of its planets, making it more difficult for them to stay in orbit. However, the star's mass and gravitational pull could also play a role in keeping the planets in orbit.

3. What factors would contribute to the stability of S5-HVS1's planets?

The stability of S5-HVS1's planets would depend on factors such as the star's mass, the distance of the planets from the star, and the strength of the star's gravitational pull. Other factors such as the presence of other nearby stars or the presence of a debris disk could also impact the stability of the planets.

4. Is it possible for S5-HVS1 to have habitable planets?

It is possible for S5-HVS1 to have habitable planets, but it would depend on a variety of factors such as the distance of the planets from the star, the presence of water and other essential elements, and the stability of the planet's orbit. The high velocity of the star could also impact the potential habitability of its planets.

5. How would the discovery of planets around S5-HVS1 impact our understanding of stellar evolution?

The discovery of planets around S5-HVS1 could provide valuable insights into the formation and evolution of stars. It could also help us better understand how planets can form and survive in extreme environments, such as around high-velocity stars. This discovery could also challenge existing theories and lead to new discoveries in the field of stellar evolution.

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