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"There's nothing to be gained scientifically from watching the orbiting systems in a time lapse video, but it helps others appreciate what we're studying," Wang says.
"It can be difficult to explain the nuances of science with words. But showing science in action helps others understand its importance."
The innermost exoplanet is HR8799e, with a mass of 7.4 Jupiters orbiting at a distance of 16.25 times the separation between Earth and the Sun, or astronomical units, for an orbital period of 45 years. Scientists have been able to analyze the light from this exoplanet to determine that it's a storm-wracked baby gas giant.
Moving outwards, HR8799d has the mass of 9.1 Jupiters, and orbits at 26.67 astronomical units for an orbital period of 100 years.
HR8799c is 7.8 Jupiters in mass, orbiting at a distance of 41.4 astronomical units (just a little wider than the separation between the Sun and Pluto) for an orbital period of 190 years. It has water in its atmosphere, scientists have found.
Finally, HR8799b clocks in at 5.7 Jupiters, with a separation of 71.6 astronomical units and an orbital period of 460 years.
www.sciencealert.com...
originally posted by: gortex
a reply to: cooperton
Perspective.
All four planets b,c,d and e have roughly though not perfectly circular orbits.
originally posted by: cooperton
originally posted by: gortex
a reply to: cooperton
Perspective.
They said themselves it's like a top-down view. Were supposedly viewing this solar system perpendicularly to its solar plane.
You're seeing in that timelapse what should approximately be the furthest distance the planet will be... you can tell because the timelapse shows that's approximately a circular trajectory that the light is taking.
I tried to look for more info, such as how they came up with the numbers but couldn't find anything. It's the classic "I made it up" argument. Trust me, I don't like ruining Santa Claus but unless there's some sort of explanation for its proximity to its sun then this is obviously not a planet. I would be open to changing my mind if there's some better reasoning behind their assumption.
originally posted by: Arbitrageur
The closest planet to the HR8799 star has a major orbital axis of at least 16 times the distance from the Earth to the sun (16.25 AU), so by earth standards it's not close to the star at all. The star is about 1.5 solar masses so significantly more massive than our sun, but not a super-massive star.
I have to guess you are somehow misinterpreting the size of the star when you look at the image in the OP.
originally posted by: tjack
a reply to: cooperton
Why would they have to block more than just the solar diameter? Simple. When you're trying to see the visible light reflected off planets over 130 light years away, you have to have the sensitivity cranked so high that you not only need to block the sun, but the corona, and as much space between the sun and the planets as possible, or the instrumentation would be overwhelmed with the extra light.
When they block our suns solar disk, its to have a clear look at the corona and other relatively nearby objects. Different situation.
You have a lot of questions but you don't seem interested in looking for answers.
originally posted by: cooperton
Why would they have to block such a larger portion in the timelapse unless that was actually the size of that solar systems sun? I'm not blindly trusting the experts anymore. They have to have an explanation, which they don't give...
originally posted by: cooperton
originally posted by: tjack
a reply to: cooperton
Why would they have to block more than just the solar diameter? Simple. When you're trying to see the visible light reflected off planets over 130 light years away, you have to have the sensitivity cranked so high that you not only need to block the sun, but the corona, and as much space between the sun and the planets as possible, or the instrumentation would be overwhelmed with the extra light.
When they block our suns solar disk, its to have a clear look at the corona and other relatively nearby objects. Different situation.
The sun doesn't light up the night sky, so why would a distant star's indirect light interfere with light detecting instruments here on earth? That black disk in the timelapse is blocking all the direct light coming from the star... which makes that the diameter of the star itself.
originally posted by: wildespace
Have a read: en.wikipedia.org...
Even solar coronographs cover more than the Sun's diameter. www.youtube.com...
The outer planet orbits inside a dusty disk like the Solar Kuiper belt. It is one of the most massive disks known around any star within 300 light years of Earth, and there is room in the inner system for terrestrial planets.[22] There is an additional debris disk just inside the orbit of the innermost planet.[8]
The orbital radii of planets e, d, c, and b are 2–3 times those of Jupiter, Saturn, Uranus, and Neptune's orbits, respectively. Because of the inverse square law relating radiation intensity to distance from the source, comparable radiation intensities are present at distances √4.9 ≈ 2.2 times farther from HR 8799 than from the Sun, the upshot being that corresponding planets in the solar and HR 8799 systems receive similar amounts of stellar radiation.[8]
en.wikipedia.org...
originally posted by: gortex
The outer planet orbits inside a dusty disk like the Solar Kuiper belt. It is one of the most massive disks known around any star within 300 light years of Earth, and there is room in the inner system for terrestrial planets.[22] There is an additional debris disk just inside the orbit of the innermost planet.[8]
The orbital radii of planets e, d, c, and b are 2–3 times those of Jupiter, Saturn, Uranus, and Neptune's orbits, respectively. Because of the inverse square law relating radiation intensity to distance from the source, comparable radiation intensities are present at distances √4.9 ≈ 2.2 times farther from HR 8799 than from the Sun, the upshot being that corresponding planets in the solar and HR 8799 systems receive similar amounts of stellar radiation.[8]
en.wikipedia.org...