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wnowak writes:
Jonathan Silverlight writes: Can you imagine the feelings of astronomers if Charon hadn't been discovered until 1990, and they realised they had missed a series of eclipses which won't recur for over a century? :-) Yes I can, because when the satellite was discovered in 1978, the orbit was known to be nearly edge on, but it was not known whether it was opening or closing, thus there was a 50 percent chance that the eclipses had been missed. Hmm ... that is in contradiction with what Stern says in his book; "... However, the fact that no observer had accidently stumbled onto one in progress hinted it was more likely that the event were in future, than in the recent past. " ( page #66 ) This suggests 50% ++, correct Mr. Tholen ? I don't buy the argument. There wasn't a whole lot of accurate photometry being done prior to the discovery of the satellite. The events themselves lasted only about five hours, and that's for a central event (less for the grazing events). With two events per orbit and one orbit every 150 hours, you're talking one part in 15. That is, if someone were making random observations, there's a 94 percent chance that the observations would be at times when no event was occurring. But as I said, there weren't a whole lot of observations being made. I'd have to dig into the literature to count the number of photometric points obtained in the 1970s, but I'd guesstimate 30. If events were occurring, that's two potential observations at the time of events. They could have been easily dismissed as bad points. Furthermore, I don't know of anybody who was taking high time resolution observations of Pluto in the 1970s. You'd need several points during an event to see the trend. A single low point could be easily dismissed as a faulty observation. Meanwhile, there is also a claim in the literature that events were seen when we now know there could not have been events, which demonstrates that faulty observations can be made. To tell you the truth I do not quite understand what Stern is talking about. For sure you know, since your picture is in the same book a few pages down the road. Please explain this to us. I hope the above is sufficient. Yes it is, and I agree 100% or to be more precise ( 50 + 50)% ![]() Talking about eclipses of PLuto and Charon, Stern says "... Then exactly- half a Charon-orbit later - 3.194 days after Binzel's first event, on February 20th, another young astronomer, the University of Hawaii's David Tholen, caught Charon falling in PLuto's shadow, ...". Binzel's and your discovery exactly 20 years ago. Happy anniversary ![]() I understand that above you are referring also to observations made a month earlier on 16th of January by Buratti and Tedesco, correct ? Those observations are more controversial. Originally it was suggested that an event had been seen, but it was later discovered that the CCD dewar had run out of liquid nitrogen and had started warming up, after which the data were considered suspect. After the time coincidence with the Feb 17 and 20 events was noticed, the Jan 16 data were once again put forward as representing an event. However, the data show an event that is deeper than the Feb 17 event, despite the fact that we now know from the orbit determination that less surface area was occulted on Jan 16 than on Feb 17 and therefore could be no deeper than the Feb 17 event. Also, the event was not very symmetrical. In other words, the data were once again considered suspect. What is certain is that observations were being made at the time of an event on Jan 16. So, we have a very precise date of the start, however the end is somehow not clear. Some sources say 1991, some other say 1990. Why is it like that ? The end was also important since it would help us to calculate the precise date of the P+CH equinox. Nobody rally cared to look for the end. People got tired ![]() Not at all. I looked for the end as vigorously as I looked for the start. They ended in 1990, twice. Prior to opposition, there were eclipse events, but eventually Pluto's heliocentric motion caused the events to end as seen from the perspective of the Sun. The Earth moved to the other side of its orbit fast enough to move back into the region where occultations could still be seen, thus events resumed after opposition, and then ended again as the Earth started back over to the other side of its orbit, moving out of the occultation region. There were no events in 1991. There were also no events near opposition in 1990. I have a lightcurve taken in May that is flat to a couple thousandths of a magnitude. They put a very tight constraint on the sizes of the two bodies. |
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Mike Dworetsky writes:
Charon is more than two magnitudes fainter than Pluto. That depends on the wavelength. In visible light, Charon is 5.5 times fainter than Pluto. That's less than two magnitudes. |
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#15
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wnowak writes:
Jonathan Silverlight writes: Can you imagine the feelings of astronomers if Charon hadn't been discovered until 1990, and they realised they had missed a series of eclipses which won't recur for over a century? :-) Yes I can, because when the satellite was discovered in 1978, the orbit was known to be nearly edge on, but it was not known whether it was opening or closing, thus there was a 50 percent chance that the eclipses had been missed. Hmm ... that is in contradiction with what Stern says in his book; "... However, the fact that no observer had accidently stumbled onto one in progress hinted it was more likely that the event were in future, than in the recent past. " ( page #66 ) This suggests 50% ++, correct Mr. Tholen ? I don't buy the argument. There wasn't a whole lot of accurate photometry being done prior to the discovery of the satellite. The events themselves lasted only about five hours, and that's for a central event (less for the grazing events). With two events per orbit and one orbit every 150 hours, you're talking one part in 15. That is, if someone were making random observations, there's a 94 percent chance that the observations would be at times when no event was occurring. But as I said, there weren't a whole lot of observations being made. I'd have to dig into the literature to count the number of photometric points obtained in the 1970s, but I'd guesstimate 30. If events were occurring, that's two potential observations at the time of events. They could have been easily dismissed as bad points. Furthermore, I don't know of anybody who was taking high time resolution observations of Pluto in the 1970s. You'd need several points during an event to see the trend. A single low point could be easily dismissed as a faulty observation. Meanwhile, there is also a claim in the literature that events were seen when we now know there could not have been events, which demonstrates that faulty observations can be made. To tell you the truth I do not quite understand what Stern is talking about. For sure you know, since your picture is in the same book a few pages down the road. Please explain this to us. I hope the above is sufficient. Yes it is, and I agree 100% or to be more precise ( 50 + 50)% ![]() Talking about eclipses of PLuto and Charon, Stern says "... Then exactly- half a Charon-orbit later - 3.194 days after Binzel's first event, on February 20th, another young astronomer, the University of Hawaii's David Tholen, caught Charon falling in PLuto's shadow, ...". Binzel's and your discovery exactly 20 years ago. Happy anniversary ![]() I understand that above you are referring also to observations made a month earlier on 16th of January by Buratti and Tedesco, correct ? Those observations are more controversial. Originally it was suggested that an event had been seen, but it was later discovered that the CCD dewar had run out of liquid nitrogen and had started warming up, after which the data were considered suspect. After the time coincidence with the Feb 17 and 20 events was noticed, the Jan 16 data were once again put forward as representing an event. However, the data show an event that is deeper than the Feb 17 event, despite the fact that we now know from the orbit determination that less surface area was occulted on Jan 16 than on Feb 17 and therefore could be no deeper than the Feb 17 event. Also, the event was not very symmetrical. In other words, the data were once again considered suspect. What is certain is that observations were being made at the time of an event on Jan 16. So, we have a very precise date of the start, however the end is somehow not clear. Some sources say 1991, some other say 1990. Why is it like that ? The end was also important since it would help us to calculate the precise date of the P+CH equinox. Nobody rally cared to look for the end. People got tired ![]() Not at all. I looked for the end as vigorously as I looked for the start. They ended in 1990, twice. Prior to opposition, there were eclipse events, but eventually Pluto's heliocentric motion caused the events to end as seen from the perspective of the Sun. The Earth moved to the other side of its orbit fast enough to move back into the region where occultations could still be seen, thus events resumed after opposition, and then ended again as the Earth started back over to the other side of its orbit, moving out of the occultation region. There were no events in 1991. There were also no events near opposition in 1990. I have a lightcurve taken in May that is flat to a couple thousandths of a magnitude. They put a very tight constraint on the sizes of the two bodies. This confirms what I have checked with HORIZONS online software. How did HORIZONS confirm when events ended (twice) in 1990? This also contradicts Stern again. He says 1991. Where does he have the data from ? He doesn't. The logical question here is; what was the date of equinox, and how precisely we know that ? 1988. A more precise date is in one of my papers, which I do not have at home. The perihelion date is stated as 5th of September 1989. I did not find the date of equinox mentioned anywhere. I recall it being mentioned in one of my AJ papers that computed when events would occur for that year. |
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wnowak writes:
Mike Dworetsky writes: Charon is more than two magnitudes fainter than Pluto. That depends on the wavelength. In visible light, Charon is 5.5 times fainter than Pluto. That's less than two magnitudes. For what value of PLuto's albedo ? Pluto's albedo is a strong function of both rotational phase and wavelength. |
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#18
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#19
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wnowak writes:
Mike Dworetsky writes: Charon is more than two magnitudes fainter than Pluto. That depends on the wavelength. In visible light, Charon is 5.5 times fainter than Pluto. That's less than two magnitudes. For what value of PLuto's albedo ? Pluto's albedo is a strong function of both rotational phase and wavelength. My point is that in 1950 the polar regions of PLuto were visible from the Earth, that are more reflective as far as I know. So, in spite of the fact that PLuto was fainter, the relative difference of brightness between two objects could have been above 2 mag. making it a bit more difficult to discover a moon. Suppose the pole of Charon is also brighter? All we know is that there isn't much variation in brightness of Charon as a function of longitude. We have practically no information on the variation in brightness as a function of latitude. Also, please remember that PLuto was farther so the max. angular distance was .... let me calculate .... ~ 0.74 arsec ? On the other hand, the minor axis of the projected orbit was larger, so Charon didn't get as close to Pluto. If these guys were not lucky, and observed at min. angular distance then it takes us down to ... ~ 0.66 * 0.74 = 0.49 ! This is probably just a bit too little. Once I have time, I will use HORIZONS again to verify for the date of 21st of March 1950, or maybe somebody else is interested in doing this. Any volunteers ? ![]() |
#20
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