C/1975 T2 (Suzuki–Saigusa–Mori)
Long-period comet discovered by five Japanese observers in 1975.
C/1975 T2 (Suzuki–Saigusa–Mori) is a long-period comet. Five Japanese observers independently spotted it on 5 October 1975. It came within 0.104 AU (15.6 million km) of Earth on 31 October 1975, becoming bright enough to see without a telescope. The comet is linked to the lambda Ursae Majorids meteor shower. The discovery happened within a half-hour window on 5 October. The five observers were Shigenori Suzuki (Aichi), Yoshikazu Saigusa (Kofu, Yamanashi), Hiroaki Mori (Mugegawa, Gifu), Kiyomi Okazaki (Kahoku, Yamagata), and Shigeru Furuyama (Tone, Ibaraki). Under international rules, only the first three discoverers whose telegrams reach the Central Bureau for Astronomical Telegrams get their names on the comet, hence Suzuki–Saigusa–Mori. Remarkably, Mori had also co-discovered another comet, C/1975 T1 (Mori–Sato–Fujikawa), 70 minutes earlier—the first time anyone found two comets in a single night. Mori used 20×120 binoculars; the others used reflector telescopes. Giovanni Casari from Novi di Modena also found the comet independently on 6 October. At discovery, the comet appeared diffuse, with no central concentration or tail, and had an apparent magnitude of 9. It showed little motion because it was heading toward Earth. After passing perihelion on 15 October, it brightened quickly and moved toward our planet, making its closest approach on 31 October. By 20 October its magnitude had reached 8. John Bortle estimated magnitude 6.8 on 22 October and 5.5 on 28 October; over that period the coma grew from 5 arcminutes (12 October) to 12 arcminutes (28 October). On 28 October Bortle also reported a tail about one degree long and a diffuse halo roughly one degree across. As the comet neared Earth, it slipped between the Sun and our planet, reaching a solar elongation of just 5 degrees on 31 October. That day, at 14:43 UTC, it passed at 0.104 AU (15.6 million km; 9.7 million mi)—the closest observed cometary approach since 1930, tied with C/1961 T1 (Seki). The comet then moved southward and was recovered on 3 November. T. Morgan at Sydney Observatory estimated magnitude 4 on 4 November. On 6 November David Seargent saw it with the naked eye, estimating magnitude 4.8. By 12 November it had faded to magnitude 7.2, and by 2 December to 9.5. The last detection came on 4 January 1976.
Quick Facts
- Discovery Ref
- IAUC_2847
- Discoverer
- Shigenori Suzuki · Yoshikazu Saigusa · Hiroaki Mori
- Discovery Site
- Japan
- Discovery Date
- 5 October 1975
- Designations
- 1975 X, 1975kICQ1
- Orbit Ref
- jpldata
- Epoch
- 31 October 1975 (JD 2442716.5)
- Observation Arc
- 90 days
- Obs
- 112
- Aphelion
- 115.6 AU
- Perihelion
- 0.838 AU
- Semimajor
- 58.2 AU
Facts from the source article.
Lore & Background
The comet was discovered independently on 5 October 1975 by five Japanese observers within 30 minutes: Shigenori Suzuki, Yoshikazu Saigusa, Hiroaki Mori, Kiyomi Okazaki, and Shigeru Furuyama. By international agreement, the comet bears the names of the three discoverers whose telegrams arrived first at the Central Bureau for Astronomical Telegrams, hence Suzuki–Saigusa–Mori. Mori had also co-discovered another comet, C/1975 T1 (Mori–Sato–Fujikawa), 70 minutes earlier, marking the first time a person discovered two comets in one night. Mori used 20×120 binoculars, while the other discoverers used reflector telescopes. The comet was also discovered independently by Giovanni Casari on 6 October. Upon discovery, the comet was described as diffuse, without central concentration or tail, with an apparent magnitude of 9. It displayed very little apparent motion as it was heading toward Earth. The comet brightened rapidly after perihelion on 15 October and moved toward Earth, with closest approach on 31 October. On 20 October its magnitude was 8; on 22 October John Bortle estimated magnitude 6.8; on 28 October he estimated magnitude 5.5, with the coma increasing from 5 arcminutes on 12 October to 12 arcminutes on 28 October. On 28 October Bortle also reported a tail about one degree long and a diffuse halo about one degree across. On 31 October the comet was at a solar elongation of 5 degrees and made its closest approach to Earth at 0.104 AU. This was, along with the equally close approach of C/1961 T1 (Seki), the closest observed approach of a comet to Earth since 1930. The comet moved southward and was recovered on 3 November. On 4 November T. Morgan estimated its magnitude at 4. On 6 November David Seargent spotted it with the naked eye at magnitude 4.8. By 12 November it had faded to magnitude 7.2, and by 2 December to 9.5. The comet was last detected on 4 January 1976.
Reader's Guide
The comet's significance lies in its close approach to Earth—0.104 AU on 31 October 1975—which, along with C/1961 T1 (Seki), was the closest observed approach of a comet to Earth since 1930. This proximity allowed it to become visible to the naked eye, with magnitude estimates as bright as 4. The comet's rapid brightening and large coma (12 arcminutes by 28 October) and tail (about one degree) made it a notable object for amateur observers. Its association with the lambda Ursae Majorids meteor shower, confirmed by numerical models and detected by the Croatian Meteor Network and SonotaCo from 2007 to 2011, adds to its legacy. The shower peaks on 28 October. The comet has also been suggested as the parent body of the October Ursae Majorids, first observed in 2006. The discovery story is remarkable: five Japanese observers independently found it within 30 minutes, and one of them, Hiroaki Mori, had discovered another comet earlier the same night—the first time a person discovered two comets in one night.
Did You Know?
- The comet was discovered by five Japanese observers within 30 minutes on 5 October 1975.
- Hiroaki Mori discovered two comets in one night, the first person to do so.
- The comet's closest approach to Earth was 0.104 AU on 31 October 1975, the closest since 1930 (along with C/1961 T1).
- The comet is associated with the lambda Ursae Majorids meteor shower, which peaks on 28 October.
Frequently Asked Questions
Who discovered C/1975 T2 (Suzuki–Saigusa–Mori)?
Five Japanese amateur astronomers independently spotted the comet within roughly thirty minutes on 5 October 1975. The observers were Shigenori Suzuki in Aichi, Yoshikazu Saigusa in Kofu, Hiroaki Mori in Mugegawa, Kiyomi Okazaki in Kahoku, and Shigeru Furuyama in Tone. Under IAU naming conventions, only the first three are credited in the official designation.
What kind of object is C/1975 T2 (Suzuki–Saigusa–Mori)?
It is a long-period comet that travels on a highly elongated orbit around the Sun, taking many years to complete one circuit. Its perihelion fell on 15 October 1975, and it reached an estimated peak apparent magnitude of 4, bright enough for unaided-eye viewing.
How close did C/1975 T2 come to Earth?
The comet passed within 0.104 AU, roughly 15.6 million kilometres, of Earth on 31 October 1975 at 14:43 UTC. At that range it was luminous enough for observers to see it clearly without a telescope.
What meteor shower is linked to C/1975 T2 (Suzuki–Saigusa–Mori)?
The comet is the parent body of the lambda Ursae Majorids meteor shower. When Earth's orbit intersects the trail of debris the comet sheds along its path, the resulting meteor activity is attributed to this object.
Why is C/1975 T2 (Suzuki–Saigusa–Mori) notable in amateur astronomy?
It is celebrated because five separate observers spread across different Japanese prefectures independently confirmed the same new comet within a single half-hour window on 5 October 1975. The episode is frequently cited as a standout example of coordinated amateur sky-watching producing a major discovery.
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