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Great Comet of 1901

Non-periodic comet

Great Comet of 1901

Summary

Non-periodic comet

FieldValue
nameC/1901 G1 (Viscara)
(Great Comet of 1901)
imageGreat comet of 1901.jpg
captionThe Great Comet of 1901 photographed by Edward Emerson Barnard on 11 May 1901
discovery_ref
discovererViscara
discovery_sitePaysandú, Uruguay
discovery_date12 April 1901
designations1901 I, 1901a
orbit_ref
epoch18 May 1901 (JD 2415522.5)
observation_arc42 days
obs54
perihelion0.245 AU
aphelion~7,100 AU
semimajor~3,500 AU
eccentricity0.99993
period~210,900 years
inclination131.077°
asc_node111.038°
arg_peri203.046°
mean0.0001°
tjup–0.402
Earth_moid0.4523 AU
Jupiter_moid0.1551 AU
physical_ref
mean_radius4.77 km
M11.7
M29.0
magnitude–1.5
(1901 apparition)
last_p24 April 1901

(Great Comet of 1901) (1901 apparition)

The Great Comet of 1901, sometimes known as Comet Viscara, formally designated C/1901 G1 (and in the older nomenclature as 1901 I and 1901a), was a non-periodic comet which became bright in the spring of 1901. Visible exclusively (or almost exclusively) from the Southern Hemisphere, it was discovered on the morning of April 12, 1901 as a naked-eye object of second magnitude with a short tail. On the day of perihelion passage, the comet's head was reported as deep yellowish in color, trailing a 10-degree tail. It was last seen by the naked eye on May 23.

Discovery and observations

In the pre-dawn of 12 April 1901 there was a naked-eye discovery of the comet by Viscara, the manager of an estancia in the Departamento de Paysandú, Uruguay. In the pre-dawn of April 23 the comet was observed in Queenstown, South Africa and on April 24 by David Gill and Robert Innes at the Royal Observatory, Cape of Good Hope; the tail was then about 10° long. On April 24 the comet was also observed at Cape Leeuwin in Western Australia. At the Sydney Observatory on April 25, H. C. Russell found the tail to be about 2° long.

The comet on May 7, 1901.

When the comet's brightness reached a maximum on May 5, the tail had fanned out with a weak plasma tail about 45° long and a curved dust tail about 15° long. On May 5 the comet's brightness reached magnitude 1 or perhaps brighter. According to some observers (of the nucleus viewed telescopically following sunrise) the brightness might have reached magnitude −1.5. From naked-eye observations on May 5 there were at least two reports of aurora-like undulations in the tail.

The comet was readily visible to the naked eye until about May 20 and visible by telescope until October.

Orbit

Using 160 observations over 43 days, Charles J. Merfield (1866–1931) could calculate only a parabolic orbit, inclined about 131° to the ecliptic. The comet travelled in a retrograde orbit relative to the planetary orbits. The comet was on April 10 about .56 AU from Venus and on April 21 about .19 AU from Mercury. On April 24 the comet reached perihelion at about .245 AU from the Sun. On April 30 the comet made its closest approach to planet Earth at about 0.83 AU.

Tebbutt's summary

In the section of his Astronomical Memoirs entitled 1901, Tebbutt wrote:

Notes

References

| access-date= 4 November 2024 }}

| trans-title= On the discovery of Comet 1901a | access-date= 23 November 2024

| doi-access= free | arxiv= 1204.2285

| bibcode-access= free | doi-access= free }}

| bibcode-access= free

| access-date= 13 September 2025 }}

| access-date= 9 November 2024 }}

| access-date= 23 November 2024 }}

| access-date= 17 June 2014 }}

| doi-access= free

| chapter-url= https://books.google.com/books?id=2FNfjWKBZx8C&pg=PA271

| bibcode-access= free | doi-access= free }}

| chapter-url= https://books.google.com/books?id=DFgMAaU3vA8C&pg=PA235

| chapter-url= https://books.google.com/books?id=XiNPAQAAIAAJ&pg=PA104 }} (Note that 23 million miles = .2474 AU.)

| archive-date= 20 December 2008 | archive-url= https://web.archive.org/web/20081220235836/http://chemistry.unina.it/~alvitagl/solex/ | url-status=dead }}

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