03-24-2005
There still seems to be quite a body of
references to counter your theory.
Quote:
The end of a short life
Eta Carinae is destined to die young. Most stars live for billions of years, but stars as massive and active as Eta Carinae burn through their fuel in an extremely short time -- as short as one million years or so, very quick for a star. They almost always end the same way: With a supernova explosion, a massive detonation that blows the star apart and scatters its remains for trillions of miles (kilometers) around.
That's how most supermassive stars end, but Eta Carinae is such an extreme case that another possibility exists: It could end as a hypernova, a super-supernova that at its peak will outshine the entire galaxy.
Chandra's X-ray image of Eta Carinae reveals a hot inner core and three distinct structures racing outward at high speeds.
The blazing violence of such an event is difficult to describe. Were it much closer it could even wipe out all life on Earth, eradicating our thin biosphere just like an ultraviolet lamp kills microbes. Fortunately it's not that close, but at 7,500 light-years it's still close enough to do some damage.
However, the likely damage is not to humans directly, but to satellites and the upper atmosphere. That's because an explosion of this type generates huge amounts of high-energy radiation such as gamma rays. We on Earth are well shielded from gamma rays by our atmosphere, but satellites in space would be vulnerable and some of their electronics could be damaged by such an event.
Some have speculated that a huge blast of gamma rays could also affect the upper atmosphere, including the ozone layer. But that remains only speculation, and any such effect is likely to be very transient because the blast of gamma rays would be fairly brief.
The only humans who might suffer directly from Eta Carinae's violent demise would be astronauts in space. Outside of the Earth's protective atmosphere they would be subject to the same powerful radiation as satellites, with conceivably lethal effect. While our own sun is also capable of lethal emissions, such as coronal mass ejections that could be harmful to astronauts, the difference is that our sun's eruptions usually give us some warning, whereas Eta Carinae would not.
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LEARN ABOUT SUNOS
mlib_volumefindmaxcmask_s16
mlib_VolumeFindMaxCMask_U8(3MLIB) mediaLib Library Functions mlib_VolumeFindMaxCMask_U8(3MLIB)
NAME
mlib_VolumeFindMaxCMask_U8, mlib_VolumeFindMaxCMask_S16 - maximum intensity searching
SYNOPSIS
cc [ flag... ] file... -lmlib [ library... ]
#include <mlib.h>
mlib_status mlib_VolumeFindMaxCMask_U8(mlib_u8 *max, const mlib_rays *rays, const mlib_u8 *cmask, mlib_s32 thresh);
mlib_status mlib_VolumeFindMaxCMask_S16(mlib_s16 *max, const mlib_rays *rays, const mlib_u8 *cmask, mlib_s32 thresh);
DESCRIPTION
Each function performs maximum intensity searching.
It uses the following equation:
max[i] = MAX{ rays->results[j][i]
j = 0, 1, ..., rays->nsteps[i]; cmask[j] > thresh }
where i = 0, 1, ..., rays->nrays - 1.
PARAMETERS
The function takes the following arguments:
max Pointer to an array of rays->nrays maximum values of the samples in each ray.
rays Pointer to an mlib_rays structure. The data rays->results are organized with ray number (rather than ray step) varying
fastest. Ray number and ray step are the output of the ray casting functions. The data might have values beyond the maximum
step on a ray. For example, rays->results[rays->nsteps[i]][i] on ray i might not equal 0.
cmask Pointer to an unsigned 8-bit mask array. If cmask[j] > thresh, then data in step j, rays->results[j], are considered.
thresh Threshold.
RETURN VALUES
The function returns MLIB_SUCCESS if successful. Otherwise it returns MLIB_FAILURE.
ATTRIBUTES
See attributes(5) for descriptions of the following attributes:
+-----------------------------+-----------------------------+
| ATTRIBUTE TYPE | ATTRIBUTE VALUE |
+-----------------------------+-----------------------------+
|Interface Stability |Evolving |
+-----------------------------+-----------------------------+
|MT-Level |MT-Safe |
+-----------------------------+-----------------------------+
SEE ALSO
mlib_VolumeFindMax_U8(3MLIB), mlib_VolumeFindMaxBMask_U8(3MLIB), attributes(5)
SunOS 5.10 10 Nov 2004 mlib_VolumeFindMaxCMask_U8(3MLIB)