QUOTE
NEMEISIS HAS A 26 MILLION YEAR ORBIT PUTTING IT A LIGHT YEAR OR TWO AWAY IN MY OPINION. THE SUPERNOVA THAT PRODUCED IT PRODUCED THE MATERIAL FOR THIS SOLAR SYSTEM. ITS AS SIMPLE AS THAT.
Orbital period is related to mean orbital distance by T^2=R^3, thus an object orbiting with a period 2.6x10^7 time that of earth would have a mean orbital distance of somewhat less than 1x10^5 AU so, a little more than 2 light-years. Supernovae are very powerful events, I don't think a gas cloud 2 light-years distant would survive. Besides, why would only the sun orbit around the supernova remnant when there are other stars at similar distances (proxima, alpha, beta Centauri).
A supernova need not be nearby to have seeded the pre-solar nebula with heavy elements. The elements produced in the supernova would travel outwards until they were stopped by something, in this case the gas and dust of the early solar system.
In addition, I don't think the sun could "hold on" to an object 2 light-years distant very effectively due to the effects of other stars and debris (in the Oort Cloud) on such objects. Keep in mind, 2+ light-years is the mean distance, objects in the Oort cloud tend to have elongated orbits that take them much closer and then much farther than their mean distances.
QUOTE (->
| QUOTE |
| NEMEISIS HAS A 26 MILLION YEAR ORBIT PUTTING IT A LIGHT YEAR OR TWO AWAY IN MY OPINION. THE SUPERNOVA THAT PRODUCED IT PRODUCED THE MATERIAL FOR THIS SOLAR SYSTEM. ITS AS SIMPLE AS THAT. |
Orbital period is related to mean orbital distance by T^2=R^3, thus an object orbiting with a period 2.6x10^7 time that of earth would have a mean orbital distance of somewhat less than 1x10^5 AU so, a little more than 2 light-years. Supernovae are very powerful events, I don't think a gas cloud 2 light-years distant would survive. Besides, why would only the sun orbit around the supernova remnant when there are other stars at similar distances (proxima, alpha, beta Centauri).
A supernova need not be nearby to have seeded the pre-solar nebula with heavy elements. The elements produced in the supernova would travel outwards until they were stopped by something, in this case the gas and dust of the early solar system.
In addition, I don't think the sun could "hold on" to an object 2 light-years distant very effectively due to the effects of other stars and debris (in the Oort Cloud) on such objects. Keep in mind, 2+ light-years is the mean distance, objects in the Oort cloud tend to have elongated orbits that take them much closer and then much farther than their mean distances.
YOU ARE WRONG. In binary systems one of the companions does not wander off. It would be gravitationally bound.
That is fallacious logic, you are saying: the sun is part of a binary system because it is part of a binary system, without giving any evidence.
Nick
7th May 2007 - 12:02 AM
HOW DID IT GET AWAY?
YOU CANNOT IGNORE THE GRAVITY HERE.
MITCH REMSCH -- LIGHT FELL --
N O M
7th May 2007 - 03:40 AM
I doubt there was just the one supernova. Gravity can cancel out when there are several massive objects around.
Also, even though the escape velocity of a neutron star may be close to lightspeed, the escape velocity required to escape the star that exploded in the supernova would have been much less. The supernova explosion would have been energetic enough to completely eject this matter.
Nick
7th May 2007 - 03:42 AM
THE GRAVITY OF THE SUN WILL KEEP NEMESIS AROUND. ITS AS SIMPLE AS THAT.
MITCH RAEMSCH -- LIGHT FELL --
N O M
7th May 2007 - 09:23 AM
QUOTE (Nick+May 7 2007, 03:42 PM)
THE GRAVITY OF THE SUN WILL KEEP NEMESIS AROUND. ITS AS SIMPLE AS THAT.
But before the sun coalesced it was a cloud of gas and dust in space. I doubt its gravity would do much to a neutron star, quite the opposite.
You seem to think the neutron star will be orbiting the sun, yet it must be many times more massive. We would be able to detect if we are orbiting a nearby (astronomically) object, even if we couldn't detect it.
Mr. Robin Parsons
7th May 2007 - 10:52 AM
at this reference
Wikipedia(dot)org it states this...
QUOTE
(SNIP) The neutron star's compactness also gives it very high surface gravity, 2×10^11 to 3×10^12 times stronger than that of Earth. (SNoP)
So you could be rather sure that if there was one anywheres near us we would have known of it by now, that and there are Luminous so they are visible in the Light spectrum, observable.
So,
no 'near Earth' Neutron Star...other then perhaps the lead singer of a Rock band
kaneda
7th May 2007 - 11:24 AM
QUOTE (N O M+May 7 2007, 10:23 AM)
But before the sun coalesced it was a cloud of gas and dust in space. I doubt its gravity would do much to a neutron star, quite the opposite.
To expand on what NOM said, the neutron star being a few times more massive than our sun would have sucked up much of the material of the solar system and possibly even what eventually formed the sun had it remained in the immediate neighbourhood.
Our sun is moving 27 miles per second towards Vega. It is possible that the other star wandered off in another direction. In theory it could be almost a third of the way to the Andromeda galaxy by now if travelling at a similar speed.
alokmohan
7th May 2007 - 01:14 PM
There is no evidence of neutron star,no pulsation.No radio wave .No evidence of nemesis.It is 10th planet or not?At least nemesis is not 10th planet.
Quantum_Conundrum
7th May 2007 - 01:24 PM
Surface gravity is irrelevant, as it does not effect gravity at a distance. Only mass effects gravity at a distance. If the sun were to instantly collapse into a black hole, there would be no gravitational effects on the earth. WE would all freeze to death within a few hours, however.
Nevertheless, a neutron star could not have been closer to the earth than several light years at ANY time in the history of the universe, or it would have destroyed the solar system.
Mr. Robin Parsons
7th May 2007 - 01:30 PM
QUOTE (Quantum_Conundrum+May 7 2007, 09:24 AM)
Surface gravity is irrelevant, as it does not effect gravity at a distance. Only mass effects gravity at a distance. If the sun were to instantly collapse into a black hole, there would be no gravitational effects on the earth. WE would all freeze to death within a few hours, however.
No ....but, as you say '
mass does' ....did you read ANY of the link?
this part perhaps
QUOTE (that Wiki Link+)
(SNIP) A typical neutron star has a mass between
1.35 to about 2.1 solar masses, (SNoP)....so if that much mass, were as close to us as the Sun currently is, now?
OldWoman1904
7th May 2007 - 01:38 PM

you guys....................
Nick
7th May 2007 - 09:58 PM
QUOTE (N O M+May 7 2007, 09:23 AM)
But before the sun coalesced it was a cloud of gas and dust in space. I doubt its gravity would do much to a neutron star, quite the opposite.
You seem to think the neutron star will be orbiting the sun, yet it must be many times more massive. We would be able to detect if we are orbiting a nearby (astronomically) object, even if we couldn't detect it.
Not so. It is orbiting so slow that it basically stays to one side of the solar system.
N O M
7th May 2007 - 10:43 PM
But it wouldn't be orbiting the sun. The sun would be orbiting it. So would several other nearby stars. We know the relative velocities of our sun and those nearby, they aren't orbiting anything.
ObservationTime
19th September 2009 - 03:15 AM
I know this argument is long over in favor of the "it just exists because it should" based on superior energy.
First an ordinary star or star cluster cannot hold onto a body with a 26 million orbit period. Other stars will gravitationally interfere. Also real orbits with 26 million year period are thousands of light years in radius. A 26 million year orbit is NOT possible for unless one object is of a mini-galaxy mass over powering influences of mere stars. Try plugging some numbers into the basic gravitational equation.
Second a neutron star in a binary system can NEVER cool off. A neutron star will FEED off the companion system HALO material, Kupiter belt, and outer planets during its closest approach. We have orbital math and countless photos of binary star interactions proving this.
A neutron star would not be "orbiting the Sun" -- basic binary star physics. Actually everything would elliptically orbit the common center of gravity (of the total system of stars and planetary disc) -- the largest stellar class objects obviously so. Smaller objects will also more obviously be orbiting closer large objects or be perturbed by by them.
Second generation stars do NOT have a a 1-to-1 relation to first generation stars. Basically new stars do not care where the dust came from. The latest evidence is that the earth has dust from 13 predecessor stars and some "virgin" primordial dust.
Nor do new stars form very close to old cores. Yes we have photos of star forming nebula that show old star cores eating up dust and preventing the formation of new stars in their immediate neighborhood. Yes we see evidence of asymmetrical nova spewing the old core out at speeds of over 1 million kilometers per hour -- meaning those cores can be far away from new stars forming in area.
Yes new star formation depends on old star cores or existing stars or novas are important to set up gravitational waves or shock waves to concentrate gas clouds -- but at a minimum 1-1/2 light year distance from existing bodies in almost all cases.
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