This paper will introduce and overview in general the
issued by the Gwansang-gam, the Astronomical Board in the Joseon Dynasty of Korea. All the Chinese characters in the 1668
was deciphered at first and these were translated into Korean and English. With these translations and the word ‘white vapor’ in particular we discuss the nature of the main object in this
. Lastly, names of observers who engaged in the observations of this 1668 celestial, which are made as a by-product of this research, are introduced.
In the course of restoration in 2011 to its original form for the copy of 「the 1668
(康熙七年星變謄錄)」, which has been kept by Nha Il-Seong since 1999, we first make an introduction to
published by the Astronomical Board (Gwansang-gam, 觀象監) of the Joseon Dynasty, 1392-1910, in order to know what kind of record this Seongbyeon Deungrok is. Then a summary to known
and the copy of the 1668
is presented. The recorded contents in this
has been deciphered, rewritten in Chinese characters, and translated to English in this paper. We point out that the record “white vapor” describes a too strange phenomenon to be a comet. It is interesting to know that an old expression of ‘Cheomseong-dae (瞻星臺)’ had been used in this
for their observing site in the North Gwangwha-bang (北部光化坊). We also present the titles and names of 12 observing staffs which were recovered by our study.
2. SEONGBYEON CHOOKHOO DANJA (星變測候單子) AND SEONGBYEON DEUNGROK (星變謄錄)
In the Joseon Dynasty, the observing staffs at the Astronomical Board (Gwansang-gam) made a report on unusual celestial and terrestrial event on their day or night duty to the Royal Secretariat (Seungjeong-won) without delay early next morning (Nha 1978). The one-page report in this process was called
Seongbyeon Chookhoo Danja
in short). The observers on duty at Cheomseong-dae worked in teams of three at normal times, with reinforcements of one or two people to make the team of four or five in a case of celestial event. If the observing staffs on duty observed an astronomical event (
, 星變), they wrote down their titles and names at the end of
before they submitted it to Seungjeong-won in the next morning. This was to make it clear that the report had been made in agreement of the observers. As a daily report,
might have been cumulated to an enormous number over ages although it may depend on the duration of each event. Once the event ended, Gwansang-gam kept the original
somewhere and made good copies of them to build a book. Titles of these books included Chinese reign names and years in those periods, and the terms
means a book and interestingly ‘Seongbyeon (星變),’ ‘Cheonbyeon (天變),’ or ‘Gaekseong (客星)’ comes before
to specify it. As an example of Chinese reign name and year, 「
The 7th year of Kangxi Seongbyeon Deungrok
(康熙七年星變謄錄)」means that it is a
made in the 7
year of the reign of Kangxi in the Qing (淸) Dynasty of China. It should be noted that they used a Chinese reign name and year in spite that it is a book written by Gwansang-gam of Joseon for a celestial event in the 9
year of the reign of Hyeonjong (1668), the 18th king in the Joseon Dynasty. There were close interchanges between the Astronomical Board Qintian-jian (欽天監) in China and Gwansang-gam (觀象監) in Joseon, and thus the same reign name was adopted in their convenience since the astronomical data exchanges were set up between the two institutions. It would be difficult to compare observing dates if different year counts are used for solar and lunar eclipses and for global events such as comets or novae (or guest stars). For example, writing the year of the celestial event in 1668 as ‘Seventh year of Kangxi’ in China on one hand but ‘Nineth year of Hyeonjong’ in Joseon on the other would have make it difficult to know that these two indicate the same event. A comparison table would have been necessary in this case. Besides, there are a number of cases that the same name was used by only one king in Korea but by several different kings through the Chinese history. For example, there was only one ‘Sejong (世宗)’ in Korea while four different kings used this name in China; 世宗 of Liao (遼), 世宗 of Jin (金),
List of Seongbyeon Deungroks.
List of Seongbyeon Deungroks.
世宗 of Ming (明), and 世宗 of Qing (淸). Considering these aspects, we may say that it was natural and reflecting an advanced form of international relationship for the two countries to have used the same reign name together. Most countries use A.D. for their dating system these days, but it was only about 110 years ago, in the 33th year of Gojong (高宗), for Joseon to have adopted A.D., a result of the import of the Gregorian calendar.
The method of recording observed comets or guest stars in
had already been established by Gwansang-gam (Seong 1818), and it is surprisingly the same as the recording way by modern astronomers. Size of a
is not clear since there remains no real copy. Only the size of a
is known to be about 20 × 34cm by measuring three
which are housed in the library of Yonsei University (Nha 1982). It should be noted that the
, which is a collection of
copies, is smaller than a
and bears the mark of being trimmed at its top and bottom in the process of bookbinding. Some characters in the top first line are partly or completely missing in some pages. Thus the vertical size of the
in Yonsei University must be larger than 35 cm at least.
3. RECOVERY OF THREE SEONGBYEON DEUNGROK (星變謄錄)
There are 8 books of
known so far. They were found and reported in Japanese to the society by Wada Yuji (和田雄治) as shown in
(Wada 1917). The existence of
became known from these
. In his article, Wada also introduced a photograph of the 1664 Kangxi (康熙)
, which contains a drawing of the comet and nearby constellations, and this is a copy of the
of the tenth day of the eleventh month (Wada 1917).
as well as
of Joseon were introduced to the world in English by the efforts of W. Carl Rufus. He presented four photographs of the drawings of the 1664 comet to Transactions of the Korea Branch of the Royal Asiatic Society which was published in 1936 (Rufus 1936). Through this paper, European people were impressed by these drawings of the comet, which had been drawn before the photographic technique was invented, and at the same time
, the collections of
, became widely known.
Over 40 years after the reports by Wada and Rufus on the eight
, the Korean society had not been aware even of the existence of the
. In the mid-1970s some people in Korea noticed at last that the all of
were missing, but fortunately during their search the last three
(Nos. 6, 7 and 8 in
) were recovered in early 1978 (Nha 1982, 1986). The library of Yonsei University purchased to possess them in no time and these three
have recently been registered as the cultural properties by the City of Seoul. This was such a gratifying event to the Korean society.
This recovery stimulated the society to search the remaining five
(Nos. 1 through 5 in
), but there was no clue to the locations of those. In the meantime, a scholar in Japan sent copies of three
(Nos. 1, 2 and 3) to one of us (Nha) at the end of 1999. It should make it clear that these are not the originals. But, this additional recovery narrowed down the missing
to Nos. 4 and 5.
4. THE CONTENTS OF THE 7TH YEAR OF KANGXI SEONGBYEON DEUNGROK (THE 1668 DEUNGROK)
The title page and contents of the
are presented in
. Except for the title page in
is a 9-page report on the observations of “white vapor” for four days from March 8, 1668 (the 26th day of the first month in the 9th year of Hyeonjong) to March 11 (the 26th day of the first month of Hyeonjong). Among those 9 pages, two pages have six Chinese characters 星變測候單子,
Seongbyeon Choohoo Danja
on upper right corner. We present in this paper the English translations from what we deciphered and translated into Korean from the 9-page report (Korea Meteorological Administration 2012). All local times corresponding to the original measurements will be quoted on the 24-hour clock. It should be noted that when quoting the 60-day cycle, pinyin has been used rather than Hangul.
Cover of the 1668 Deungrok (from Korea Meteorological Administration 2012).
Page 1 of the 1668 Deungrok (from Korea Meteorological Administration 2012).
Page 2 of the 1668 Deungrok (from Korea Meteorological Administration 2012).
Page 3 of the 1668 Deungrok (from Korea Meteorological Administration 2012).
Page 4 of the 1668 Deungrok (from Korea Meteorological Administration 2012).
Page 5 of the 1668 Deungrok (from Korea Meteorological Administration 2012).
Page 6 of the 1668 Deungrok (from Korea Meteorological Administration 2012).
Page 7 of the 1668 Deungrok (from Korea Meteorological Administration 2012).
Page 8 of the 1668 Deungrok (from Korea Meteorological Administration 2012).
Page 9 of the 1668 Deungrok (from Korea Meteorological Administration 2012).
- 4.1 Contents ofFig. 2
On the 26th day, yichou
, of this first month (of the 9th year of King Hyeonjong) (= 8 March 1668), at the beginning of dusk, one streak of white vapor arose from the western horizon and pointed towards the zenith. Its shape resembled a broom star and its tail was several jang in length and more than a cheok in width. When night came, after the third jeom [= division] of the first gyeong (= night watch), it disappeared in the west following the motion of the sky.
An official on duty deposited an observational report at the gates of the Seungjeong-won and the Sigang-won. When the gates were opened, Hui (a high-ranking official whose full name is currently uncertain) submitted the report to Yeongsa-Jejo (an official of highest rank). Officials on duty were Yoon Seong-sam, Yi Jin-ok and Jeong Deok-je.
- 4.2 Contents ofFig. 3
On the 27th day, bingyin
, of this first month (of the 9th year of King Hyeonjong) (= 9 March 1668), at night, in the first gyeong, one streak of white vapor arose from the turbid air on the western horizon and pointed towards the zenith. Its length was almost three jang and its width more than a cheok. After the fourth jeom it disappeared in the west following the motion of the sky. Since this type of phenomenon has not yet been seen before, it is impossible to give it a name.
An official on duty deposited an observational report at the gates of the Seungjeong-won and the Sigang-won. When the gates were opened, the report was delivered to Yeongsa-Jejo. The official Kim Go-seong made the observations along with other court observers.
On the same day, Yeongjeob Dogam (an official whose duty was to greet foreign ambassadors), was asked by a high-ranking official of the foreign representatives what kind of portent it could be. Yeongjeob Dogam replied that they should wait until next day and ask the staff of the Court Observatory.
At the second gyeong (20.7-22.9 h), his Royal Highness gave his assent.
- 4.3 Contents ofFig. 4
On the 28th day (= 10 March 1668), before dawn, a member of the Observatory staff Whang Hyo-gong was called to His Royal Highness and said that this (phenomenon) was a sign of drought. Whang Hyo-gong suggested addressing the foreign representative after the sacrifice. The foreign representative said that he was aware of it already. The Court Observatory staff expressed the wish that celestial portents should not be divulged to foreigners. The interpretation of this sign was based on the experience of an elderly man.
On the same day, Yeongsa-Jejo Hui said that the white vapor in the western direction appeared two nights ago at the beginning of dusk near the sunset point. However, trees of private houses close to the Observatory made celestial observation difficult. Therefore it was proposed to send observers to the top of Mt. Namsan to make their observation.
His Royal Highness gave his assent.
4.4 Contents ofFig. 5
In the evening of the same day the Jeongwon (the name of another office) reported to His Royal Highness with reference to a short report which had been received, stating that although the Observatory needed to have a clear view, the nearby trees obscured the view. These trees had not been cut back for several years, so that the observers made their observations at the house of Rangseon-goon (a grandson of King Seonjo). Therefore it was proposed to cut back the trees to facilitate observation.
His Royal Highness gave his approval to the Mayor. Next day, officials of the northern section cut back all the trees surrounding the Observatory.
- 4.5 Contents ofFig. 6
On the 28th day, dingmao
, of the first month (= 10 March 1668), at the first gyeong of the night, a streak of white vapor arose from the western horizon. It passed under (the constellation) Cheon-gun and pointed towards the second star of (the constellation) Cheon-won. Its length was about 3 jang and its width more than a cheok. Its shape resembled a broom. After the fourth jeom, following the motion of the sky it set in the west. Since this type of phenomenon has not yet been seen before, it is impossible to give it a name.
The official Kim Go-seong made this observation, together with other court observers.
- 4.6 Contents ofFig. 7
at Mt. Namsan.
In the evening of the 28th day, dingmao
, of this first month (= 10 March 1668), from the top of Mt. Namsan, after sunset and beginning with the first appearance of the stars, a white vapor was seen to arise from the western horizon. It passed under (the constellation) Cheon-gun and pointed towards the second star of (the constellation) Cheon-won. Its length was about 3 jang and its width more than a cheok. Its shape resembled a broom, but its head was invisible because of its location below the turbid horizon. At the fourth jeom of the first gyeong (20.0 h) it set on the western horizon. Since this type of phenomenon has not yet been seen before, it is impossible to give it a name.
The official Kim Go-seong made this observation, together with other court observers: Song Seom, Yoon Seong-sam, Nam Mong-sam.
- 4.7 Contents ofFig. 8
On the morning of the 29th day (= 11 March 1668), at the double hour si (= 9-11 h), the Director of the Observatory ordered two officials, Whang Hyo-gong and Seong Hoo-gwan, to jointly make observations on the mountain at Gangwha Island; they were to be accompanied by a servant, Han Geom. Now the Ministry of Defence offered horses for the two officials. They were also to be provided with necessities at the local stations on their way.
- 4.8 Contents ofFig. 9
On the 29th day, wuchen
, of this first month (= 11 March 1668), at the first gyeong of the night, a streak of white vapor arose from the western horizon. It passed the second star of (the constellation) Cheon-won, and pointed towards (the constellation) Gujusoogu. Its length was more than 5 jang and its shape resembled a broom. After the fifth jeom it set on the western horizon. Since this type of phenomenon has not yet been seen before, it is impossible to give it a name. The official Kim Go-seong made this observation, together with other court observers.
- 4.9 Contents ofFig. 10
at Mt. Namsan
In the evening of the 29
, of this first month (= 11 March 1668), (we) climbed up Mt.Namsan again and made observations. The shape of the white vapor remained the same as on the previous night, but its head was invisible because of its location below the turbid horizon. Its tail became slightly longer and passed the second star of (the constellation) Cheon-won and pointed towards (the constellation) Gujusoogu. After the fifth jeom of the first gyeong it set on the western horizon.
According to the text above, in the first day of observation, the observing staffs of Gwansang-gam named the observed celestial event ‘white vapor (白氣),’ but they called it a ‘comet’ at their report since they were not able to figure it out what the white vapor really was. However, they began to regard the white vapor as a strange phenomenon on the next day and then on. If this white vapor had been a comet, there should have been its head, but it was out of sight under the horizon. In their expression at that time, a head of comet was geunjeo(根抵, head). Thus, in search for the head of comet, they made efforts of cutting nearby trees to get better views to the horizon, and climbing up to the Mt. Namsan and even sending observing staffs to Ganghwa Island where the sight to the western horizon is guaranteed. However, they failed to find the head after all and made a conclusion saying “We are not able to name it since there has never been such a phenomenon as this.”
In the case that the head of comet is not seen even though its tail is long above the western horizon, the part of head might be located on the other side of the sun. Then, the head of this comet would be observable at the eastern horizon at dawn, instead of in the western sky in the early evening. However, they were not able to find the head in the east at dawn.
What indeed was this white vapor which they could not determine at that time? We introduce here another record from the Annals of Hyeonjong before continuing to the next section.
Jeong Tae-hwa, the prime minister, said secretly, “I heard that the Chinese envoy (北使) had noticed the extraordinary event of white vapor at night and today he was going to ask a staff of our Board of Astronomy about what this event would be an omen of. I am not sure what sign this extraordinary event is, but I suspect that it might be a portent of a war. As we cannot let the Chinese envoy (北使) know that as it is, it would be better to tell him that it is an omen of famine.”, but the king said “I don’t think we can hide the fact since they also have astronomers, but it is fine to talk to him based on what you said.” (Annals of Hyeonjong; the 28thday of the 1stmonth).
5. WHAT WAS THE WHITE VAPOR IN THE 1668 SEONGBYEON DEUNGROK?
Wada Yuji (和田雄治) is the first one who mentioned briefly the
1668 Seongbyeon Deungrok
. He introduced the celestial event as follows.
Now we examine the article of this
with 9 pages in total.
First, it cannot be a comet or guest star according to the expression in the record. It is because there repeats several times the sentence “而未見其本故不得作名” which means “Since this type of phenomenon has not yet been seen before, it is impossible to give it a name.” Among the observing staffs on that occasion, more than a few of them must have participated also in the observations of the great comet in 1664 which is a historical comet having appeared just four years before. And such observers confessed that they could not name it comet or guest star.
Second, it is stated that the tail was as long as five jangs (丈), and such a big comet cannot be imagined (Nha 1981). The greatest comet known so far is the one recorded in The 3rd year of Kangxi (康熙)
(1664), of which the tail was about two jangs (丈) long and 8 or 9 chons (寸) wide at its maximum size. The comet in The 24th year of Qianglong (乾隆)
(1759)is the famous Comet Halley, and the maximum length of its tail was only two cheoks (尺) which is less than one-tenth of the former one.
Angular sizes (角度) are used in principle for the length or width of a comet, but length units such as jang (丈), cheok (尺), or chon (寸) were used in the old literature. Converting those length units to angular sizes in degree (度) was done by Sekiguchi Rigichi (關口鯉吉), and he determined one cheok to be about one degree based on his comparison between comet drowings and records on length of tail (尾長) in several
. [Annotation: this conversion is in the paper of Sekiguchi reported to
(天文月報) of the Astronomical Society of Japan in 1910s, which has not yet been found.] Recently Nha (1981) tried another conversion of cheok for lengths of comet tails to angular sizes. Nha used two samples. First, with four photographs of the comet in
The 1664 Cheonbyeon Deungrok
, he determined about 1.5 degree for one cheok. This is a conversion factor for the 1664 comet in the period of Hyeonjong. With a set of five drawings of the comet in the 24th year of Qianglong (乾隆)
(乾隆二十四年己卯星變謄錄) which was recorded after almost 100 years from that point, however, one cheok was appeared to be 7 or 8 degrees. This is for Comet Halley in the 35th year of Youngjo (1759), but the value derived from those drawings is too large and unrealistic for acceptance. Using the factor of 1.5 degree/cheok, the length in question of in the record on ‘the 29th day of the first month, i.e. March 11, 1668,’ is converted into larger than 75 degrees. Then it is too long to be a tail of comet since this length is across almost a half of the sky. With the factor of 7-8 degrees/cheok from the period of Youngjo, it would be 350 to 400 degrees. This value is very unlikely and thus drawings in
do not represent the true length of comet tails.
Third, what seems even stranger is that the celestial event was expressed as ‘white vapor (白氣).’ There are some cases of writing color of a comet as ‘white’ but there is no other record of ‘white vapor.’ This ‘white vapor’ is certainly not a guest star. Guest star is a word for nova or supernova, but even the greatest supernova could not be seen as wide
Especially in the record of 「The 7th year of Kangxi」, “They cut the trees around Cheomseong-dae since the forest was thick and blocked the sight, observed at the summit of Mt. Namsan, and also sent an observing staff to Ganghwa Island for observations.” (omitted)
They found it in Europe on March 5 in that year, and it was a comet.
Location and shape of “white vapor (白氣)” described in the Eryue Zhongxing-tu (二月中星圖) of Yuan Qi (袁啓)’s Tianwen Tushuo (天文圖說).
spread as in this case. If it is neither a guest star nor a comet, then what is the ‘white vapor’?
The position of the ‘white vapor’ is presented in the
on the 28th day of the first month(March 10, 1668) as ‘It passed under (the constellation) Cheon-gun and pointed towards the second star of (the constellation) Cheon-won’ according to the observing records at Cheomseong-dae on Mt. Namsan. We draw the ‘white vapor’ based on its position with respect to the constellations on a star-map. The star-map used here is the
(天文圖說) by Yuan Qi (袁啓) (Yuan 1632). This map was published in the period of the Qing dynasty which is close to the occurrence of the present ‘white vapor.’
Another star-map, the
Sinbeob Nuju Tongui
(Gwansang-gam 1789), is known as a meridian star-map in Joseon Dynasty. But this map was not used because it has bright stars only and thus the faint constellations ‘Cheon-gun’ and ‘Cheon-won’ are missing in this map. On the other hand, the meridian star-map by Yuan lacks accuracies of the relative positions of the constellations whose shapes were even drawn roughly and arbitrarily. Nevertheless, as is shown in
, we draw the ‘white vapor’ on Yuan’s star-map according to the positions from the
. This position and shape of the ‘white vapor’ may not represent the real situation, but would be enough to show the phenomenon appearing very close to the horizon on the sky.
Fourth, it is hardly probable, but could we assume that the ‘white vapor’ was an aurora borealis? As aurora is an atmospheric phenomenon observable around the poles of the earth magnetic field (地球磁氣), i.e. in high latitude regions near to the north pole. Scientifically considered, aurora is not observable in Hanyang (Seoul) even towards the lowest altitudes to the horizon. Furthermore, the strongest evidence against the assumption of aurora is the record that it was seen towards the western horizon (西方天際). If the ‘white vapor’ had been an aurora, it must have been seen towards the northern horizon, but there is no record in the
to support it. Also it says that the ‘white vapor’ set in the west over time. Therefore, the ‘white vapor’ cannot be an aurora at all.
Records of the
in the possession of Nha last only four days from 26th to 29th of January on the lunar calendar. It may be probable that the original
does not end at January 29 but continuing on for at least several more days, and the later parts should have excluded from the copy-making. When they close a series of each celestial event, it was a customary practice of
in Joseon to state that the event had been concluded and to list at the end of the
all names of the observing staffs participated. Unfortunately this important part is missing in the copies of Nha.
6. EXAMINATIONS AND NEW FACTS
Lynn (1882) re-examined several observing reports available in Europe on this ‘celestial event’. The observations were performed in 1668 in various places such as Lisbon, Cape of Good Hope, Goa, San Salvador, etc., but in his brief report, Lynn paid more attention to the observational record by Father Valentin Estancel (1674) at San Salvador. Some parts of Lynn’s article are introduced here as follows.
Lynn followed up with that the perihelion distance of this comet was reported by Henderson to be 0.25113 AU. Considering that the perihelion distance of Mercury is 0.307 AU, this comet entered into the orbit of Mercury.
There is another supporting article, and according to this
“The comet was observed for a few days, commencing on the 5th of March. He saw it in the evening, and was surprised to find it of extraordinary brightness when first seen, and then decreasing, instead of becoming brighter by degrees as he had noticed in other comets. As to the color of this comet, it was at first very splendid, but the brightness lasted only for three days, after which it did considerably decay. But that which seemed somewhat strange was, that having lost so much of its light, yet its bulk was diminished, but continued rather increasing until the comet disappeared.”
The above statement, ‘he
was a comet’, is indeed a sentence by Cassini who left his mark on the history of astronomy as an excellent observer. And the statement ‘the head was either hidden by “horizontal clouds” or still below the horizon’ is completely consistent with the record by Gwansang-gam on 10th and 11th of March. With an insight on the situation, Lynn made a conclusion at the end of his article introduced above as “Any attempt to identify the comets of (omitted) with that of 1668 can be but of little weight.” This shows well that this ‘celestial event’ was regarded as extraordinary also in Europe. Considering those opinions together, we understand better the difficulties that the observing staffs at Gwansang-gam had at that time.
Also in China, there are records of celestial events written in a period close to the occurrence of the ‘white vapor.’ Here we count dates on the solar calendar. First, there is a record on a comet from January 14 to February 11 in 1668 (Beijing Observatory 1989a), but this has nothing to do with the ‘celestial event’ in question. The second record was made after about one month, on March 2, 1668. It says ‘A comet appeared at night in the west. The length of its tail was a few jangs, and it disappeared after several days’ (Beijing Observatory 1989b). This is clearly a record of comet. However, also in China, there are more than a few dozens of observing records on ‘white vapor’ and ‘black vapor (黑氣)’ during the same period. The first one on March 3 says ‘Vapor appeared in the west, which was red then looked white. The bottom of it was ‘black vapor’ and its shape is similar to a cloth (布)’ (Beijing Observatory 1989c). After this record, there are a number of records from March 6 using only the term ‘white vapor.’ Two examples are as follows. ‘(March 6): White vapor appeared with a shape like white silk (煉), which passed through the southwest and pointed straight to the northeast’ (Beijing Observatory 1989c) or ‘(March 7): White vapor like a spear (槍) appeared in the west at the 19th of the 24 periods of the day, and black vapor like a sword (刀) with three blades appeared at the night of 27th day’ (Beijing Observatory 1989d). Such Chinese records are interesting, but on the other hand, are difficult to interpret since they did not describe the shapes and positions scientifically, not like the records by the observing staffs at Gwansang-gam of Joseon.
Now we return to the records in Joseon. In addition to the
, there are other records on the ‘white vapor’ also in
(承政院日記). Among those records, the following three records in
should need new attentions.
No details were provided, but later orbits indicated the comet was then in Cetus and it was probable that only the tail was seen. The comet had passed only 1˚.5 from the sun on February 29. -------------- Giovanni Cassini obtained his first observation on the 10th (= 28th day of the first month) during the first hour of the night and saw a “path of light” which he presumed was a comet, extending from Cetus through Eridanus. The tip of the tail lay near 14 Eridani, while the head was either hidden by “horizontal clouds” or still below the horizon.
Except for 1) above, those records are against the assumption of comet. Therefore, it is clear that the 1668 celestial event is a new sample for studies on the solar activity and abnormal phenomena of the earth atmosphere. It might be such an important discovery in the ancient observing records in China, Korea, and Japan as the facts that sunspots were observed with the unaided eye and that guest stars were supernovae which made significant impacts on modern science.
As briefly mentioned earlier, there is an interesting article in the
on the 28th day of the first month in the 9th; ‘---stating that although the Cheomseong-dae needed to have a clear view, the nearby trees obscured the view. These trees had not been cut back for several years, so that the observers made their observations at the house of Rangseon-goon.’ We became aware from this article that the observing site in Hanyang at that time was North Gwangwha-bang (北部廣化坊) which is to the west of the main gate of the Changdeok Palace and in front of the current office building of . This observing site was named Gwancheon-dae (觀天臺) in 1983, about 30 years ago by Jeon & Nha (1983). However, this place should now be rightly called Cheomseong-dae in North Gwangwha-bang (北部廣化坊瞻星臺) since the old name was given without clear references at that time. At the same time, also the name of Gwancheon-dae in the Changgyeong Palace should be corrected to be Cheomseong-dae. Rangseon-goon (朗善君) is a grandson of King Seonjo and was famous as a writer. The location of
1) On the 4th and 5th days of the second month in the 9th year of Hyeonjong, the expression of chiugi (蚩尤旗)’ was used. This is an expression for a comet splitting into two tails.
2) On the 4th day of the second month in the 9th year of Hyeonjong, an unbelievable tail of 7 jangs long, which was longer than 5 jangs in theDeungrok, was observed.
3) On the 5th day of the second month in the 9th year of Hyeonjong and several days afterward, a ‘light’ was introduced as ‘vapor like fire light (有氣如火光).’
Names of the 12 Chookhoo-gwan (測候官, astronomers).
Names of the 12 Chookhoo-gwan (測候官, astronomers).
Cheomseong-dae is now clear considering that he lived in this North Gwangwha-bang.
The recovery of the 12 observing staffs in total is also a significant result. Among them, 8 were found in the
and 4 in
, whose titles and names are listed in
. It would be one of future work to determine who were participated in the comet observation four years before, the 5th year of Hyeonjong.
This work was funded by the Korea Meteorological Administration Research and Development Program under Grant RACS_2011-4016. We wish to express our sincere appreciation to Professor Richard Stephenson of University of Durham and Dr. Youngsin Chun of National Institute of Meteorological Research for their valuable advices and suggestions during the course of this research. The authors also gratefully acknowledge two anonymous referees.
Anhuisheng Shidaixuan-zhi, 2, 19, Zhongguo gudai tianxiang jiluzongji
Guangdongsheng Chaozhoufu-shi, 11, 30, Zhongguo gudai tianxiang jiluzongji
Hubeisheng Dongyangsheng-zhi, 1, 38, Zhongguo gudai tianxiang jiluzongji
GuangxishengQinzhou-zhi, 10, 19, Zhongguo gudai tianxiang jiluzongji
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