Meteor showers from known long-period comets
What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras fo...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Jenniskens, Peter [verfasserIn] |
|---|
| Format: |
E-Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2021transfer abstract |
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| Übergeordnetes Werk: |
Enthalten in: Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users - Mathew, Rajeev ELSEVIER, 2018, international journal of solar system studies, Orlando, Fla |
|---|---|
| Übergeordnetes Werk: |
volume:365 ; year:2021 ; day:1 ; month:09 ; pages:0 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.icarus.2021.114469 |
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| 520 | |a What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. | ||
| 520 | |a What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. | ||
| 700 | 1 | |a Lauretta, Dante S. |4 oth | |
| 700 | 1 | |a Towner, Martin C. |4 oth | |
| 700 | 1 | |a Heathcote, Steve |4 oth | |
| 700 | 1 | |a Jehin, Emmanuel |4 oth | |
| 700 | 1 | |a Hanke, Toni |4 oth | |
| 700 | 1 | |a Cooper, Tim |4 oth | |
| 700 | 1 | |a Baggaley, Jack W. |4 oth | |
| 700 | 1 | |a Howell, J. Andreas |4 oth | |
| 700 | 1 | |a Johannink, Carl |4 oth | |
| 700 | 1 | |a Breukers, Martin |4 oth | |
| 700 | 1 | |a Odeh, Mohammad |4 oth | |
| 700 | 1 | |a Moskovitz, Nicholas |4 oth | |
| 700 | 1 | |a Juneau, Luke |4 oth | |
| 700 | 1 | |a Beck, Tim |4 oth | |
| 700 | 1 | |a De Cicco, Marcelo |4 oth | |
| 700 | 1 | |a Samuels, Dave |4 oth | |
| 700 | 1 | |a Rau, Steve |4 oth | |
| 700 | 1 | |a Albers, Jim |4 oth | |
| 700 | 1 | |a Gural, Peter S. |4 oth | |
| 773 | 0 | 8 | |i Enthalten in |n Academ. Press |a Mathew, Rajeev ELSEVIER |t Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users |d 2018 |d international journal of solar system studies |g Orlando, Fla |w (DE-627)ELV000289655 |
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10.1016/j.icarus.2021.114469 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001548.pica (DE-627)ELV054224314 (ELSEVIER)S0019-1035(21)00150-0 DE-627 ger DE-627 rakwb eng 570 VZ BIODIV DE-30 fid 44.94 bkl Jenniskens, Peter verfasserin aut Meteor showers from known long-period comets 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. Lauretta, Dante S. oth Towner, Martin C. oth Heathcote, Steve oth Jehin, Emmanuel oth Hanke, Toni oth Cooper, Tim oth Baggaley, Jack W. oth Howell, J. Andreas oth Johannink, Carl oth Breukers, Martin oth Odeh, Mohammad oth Moskovitz, Nicholas oth Juneau, Luke oth Beck, Tim oth De Cicco, Marcelo oth Samuels, Dave oth Rau, Steve oth Albers, Jim oth Gural, Peter S. oth Enthalten in Academ. Press Mathew, Rajeev ELSEVIER Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users 2018 international journal of solar system studies Orlando, Fla (DE-627)ELV000289655 volume:365 year:2021 day:1 month:09 pages:0 https://doi.org/10.1016/j.icarus.2021.114469 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U FID-BIODIV SSG-OLC-PHA 44.94 Hals-Nasen-Ohrenheilkunde VZ AR 365 2021 1 0901 0 |
| spelling |
10.1016/j.icarus.2021.114469 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001548.pica (DE-627)ELV054224314 (ELSEVIER)S0019-1035(21)00150-0 DE-627 ger DE-627 rakwb eng 570 VZ BIODIV DE-30 fid 44.94 bkl Jenniskens, Peter verfasserin aut Meteor showers from known long-period comets 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. Lauretta, Dante S. oth Towner, Martin C. oth Heathcote, Steve oth Jehin, Emmanuel oth Hanke, Toni oth Cooper, Tim oth Baggaley, Jack W. oth Howell, J. Andreas oth Johannink, Carl oth Breukers, Martin oth Odeh, Mohammad oth Moskovitz, Nicholas oth Juneau, Luke oth Beck, Tim oth De Cicco, Marcelo oth Samuels, Dave oth Rau, Steve oth Albers, Jim oth Gural, Peter S. oth Enthalten in Academ. Press Mathew, Rajeev ELSEVIER Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users 2018 international journal of solar system studies Orlando, Fla (DE-627)ELV000289655 volume:365 year:2021 day:1 month:09 pages:0 https://doi.org/10.1016/j.icarus.2021.114469 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U FID-BIODIV SSG-OLC-PHA 44.94 Hals-Nasen-Ohrenheilkunde VZ AR 365 2021 1 0901 0 |
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10.1016/j.icarus.2021.114469 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001548.pica (DE-627)ELV054224314 (ELSEVIER)S0019-1035(21)00150-0 DE-627 ger DE-627 rakwb eng 570 VZ BIODIV DE-30 fid 44.94 bkl Jenniskens, Peter verfasserin aut Meteor showers from known long-period comets 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. Lauretta, Dante S. oth Towner, Martin C. oth Heathcote, Steve oth Jehin, Emmanuel oth Hanke, Toni oth Cooper, Tim oth Baggaley, Jack W. oth Howell, J. Andreas oth Johannink, Carl oth Breukers, Martin oth Odeh, Mohammad oth Moskovitz, Nicholas oth Juneau, Luke oth Beck, Tim oth De Cicco, Marcelo oth Samuels, Dave oth Rau, Steve oth Albers, Jim oth Gural, Peter S. oth Enthalten in Academ. Press Mathew, Rajeev ELSEVIER Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users 2018 international journal of solar system studies Orlando, Fla (DE-627)ELV000289655 volume:365 year:2021 day:1 month:09 pages:0 https://doi.org/10.1016/j.icarus.2021.114469 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U FID-BIODIV SSG-OLC-PHA 44.94 Hals-Nasen-Ohrenheilkunde VZ AR 365 2021 1 0901 0 |
| allfieldsGer |
10.1016/j.icarus.2021.114469 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001548.pica (DE-627)ELV054224314 (ELSEVIER)S0019-1035(21)00150-0 DE-627 ger DE-627 rakwb eng 570 VZ BIODIV DE-30 fid 44.94 bkl Jenniskens, Peter verfasserin aut Meteor showers from known long-period comets 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. Lauretta, Dante S. oth Towner, Martin C. oth Heathcote, Steve oth Jehin, Emmanuel oth Hanke, Toni oth Cooper, Tim oth Baggaley, Jack W. oth Howell, J. Andreas oth Johannink, Carl oth Breukers, Martin oth Odeh, Mohammad oth Moskovitz, Nicholas oth Juneau, Luke oth Beck, Tim oth De Cicco, Marcelo oth Samuels, Dave oth Rau, Steve oth Albers, Jim oth Gural, Peter S. oth Enthalten in Academ. Press Mathew, Rajeev ELSEVIER Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users 2018 international journal of solar system studies Orlando, Fla (DE-627)ELV000289655 volume:365 year:2021 day:1 month:09 pages:0 https://doi.org/10.1016/j.icarus.2021.114469 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U FID-BIODIV SSG-OLC-PHA 44.94 Hals-Nasen-Ohrenheilkunde VZ AR 365 2021 1 0901 0 |
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10.1016/j.icarus.2021.114469 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001548.pica (DE-627)ELV054224314 (ELSEVIER)S0019-1035(21)00150-0 DE-627 ger DE-627 rakwb eng 570 VZ BIODIV DE-30 fid 44.94 bkl Jenniskens, Peter verfasserin aut Meteor showers from known long-period comets 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. Lauretta, Dante S. oth Towner, Martin C. oth Heathcote, Steve oth Jehin, Emmanuel oth Hanke, Toni oth Cooper, Tim oth Baggaley, Jack W. oth Howell, J. Andreas oth Johannink, Carl oth Breukers, Martin oth Odeh, Mohammad oth Moskovitz, Nicholas oth Juneau, Luke oth Beck, Tim oth De Cicco, Marcelo oth Samuels, Dave oth Rau, Steve oth Albers, Jim oth Gural, Peter S. oth Enthalten in Academ. Press Mathew, Rajeev ELSEVIER Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users 2018 international journal of solar system studies Orlando, Fla (DE-627)ELV000289655 volume:365 year:2021 day:1 month:09 pages:0 https://doi.org/10.1016/j.icarus.2021.114469 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U FID-BIODIV SSG-OLC-PHA 44.94 Hals-Nasen-Ohrenheilkunde VZ AR 365 2021 1 0901 0 |
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Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users |
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Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users |
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meteor showers from known long-period comets |
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What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. |
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What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. |
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What long-period comets with orbital periods >250 years cause detectable meteor showers on Earth? Low-light video cameras are used to track the motion of +4 to −5 magnitude meteors in our atmosphere by triangulation and calculate the meteoroid orbit in space. In recent years, the CAMS (Cameras for Allsky Meteor Surveillance) low-light video camera network was greatly expanded and, together with other video networks, now has increased the total video meteoroid orbit database to over 2.2 million orbits. Here, we searched this database for meteor showers associated with known long-period comets. Previously, five associations were known. Now, we find 14, as well as six uncertain but likely associations. These showers show a change of longitude of perihelion with node that is a strong function of inclination. Showers of longer duration show a steeper magnitude distribution index, presumably due to aging of the meteoroid population. Showers are generally detected only if the orbital period of the comet is less than 4000 years and the Earth-Comet orbital miss distance is ≤0.10 AU. The lack of an associated meteor shower sets lower limits on the orbital period of poorly observed comets. |
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Lauretta, Dante S. Towner, Martin C. Heathcote, Steve Jehin, Emmanuel Hanke, Toni Cooper, Tim Baggaley, Jack W. Howell, J. Andreas Johannink, Carl Breukers, Martin Odeh, Mohammad Moskovitz, Nicholas Juneau, Luke Beck, Tim De Cicco, Marcelo Samuels, Dave Rau, Steve Albers, Jim Gural, Peter S. |
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