 | |
| Discovery | |
|---|---|
| Discovered by |
LINEAR 1.0-m reflector [1] |
| Discovery date | 3 February 2004 (asteroidal) 30 March 2004 (tail) |
| Designations | |
| 2004 CB | |
| Orbital characteristics | |
| Epoch | 2014-May-23 ( JD 2456800.5) [2] |
| Aphelion | 4.952 AU (Q) |
| Perihelion | 0.9695 AU (q) |
| Semi-major axis | 2.961 AU (a) |
| Eccentricity | 0.67258 |
| Orbital period | 5.09 yr |
| Inclination | 21.243° |
| Last perihelion | 2019-Jun-12
[2] 2014-May-06 [3] 2009-Apr-15 [3] |
| Next perihelion | 2024-Jul-14 [4] |
| Earth MOID | 0.05 AU (7,500,000 km) [5] |
| Physical characteristics | |
| Dimensions | 3.9 × 2.7 × 2.6 km [6] |
| 10.9 hours [7] | |
|
Comet total magnitude (M1) | 18.1 [5] |
209P/LINEAR is a periodic comet with an orbital period of 5.1 years. The comet has extremely low activity for its size and is probably in the process of evolving into an extinct comet. [6]
Observational history
The comet discovered on 3 February 2004 by Lincoln Near-Earth Asteroid Research (LINEAR) using a 1.0-metre (39 in) reflector. [1] Initially it was observed without a coma and named 2004 CB as a minor planet or asteroid, but in March 2004 Robert H. McNaught observed a comet tail which confirmed it as a comet. [8] It was given the permanent number 209P on 12 December 2008 as it was the second observed appearance of the comet. [9] Prediscovery images of the comet, dating back to December 2003, were found during 2009. [8]
209P/LINEAR came to perihelion (closest approach to the Sun) on 6 May 2014. [3] On 29 May 2014 the comet passed 0.0554 AU (8,290,000 km; 5,150,000 mi) from Earth, [5] but only brightened to about apparent magnitude 12. [10] The 2014 Earth approach was the 9th closest known comet approach to Earth. [11] The close approach allowed the comet nucleus to be imaged by Arecibo, producing the most detailed radar image of a comet nucleus to that date. [12] The radar imaging showed the comet nucleus is elongated and about 2.4 km by 3 km in size, [12] later refined to 3.9 × 2.7 × 2.6 km. [6] No evidence of large dust particles were detected in the coma. [7] The comet also had very low water production, (2.5±0.2)×1025 mol/s, from an active area measuring just 0.007 km². [6]
209P/LINEAR was recovered on 31 December 2018 at magnitude 19.2 by Hidetaka Sato. [13]
Associated meteor showers
Preliminary results by Esko Lyytinen and Peter Jenniskens, later confirmed by other researchers, predicted [14] [15] [16] 209P/LINEAR might a big meteor shower which would come from the constellation Camelopardalis on the night of 23/24 May 2014. It was possible that there could be 100 to 400 meteors per hour. [14] All the trails from the comet from 1803 through 1924 were expected to intersect Earth's orbit during May 2014. [14] The peak activity was expected to occur around 24 May 2014 7h UT when dust trails produced from past returns of the comet could pass 0.0002 AU (30,000 km; 19,000 mi) from Earth. [16] The 2014 Camelopardalids only generated 10–15 visual meteors per hour. [17] [18] But the expected radiant and date of visual maximum were correctly predicted. [18] The shower peaked around 6h UT on 24 May 2014. [18] The Canadian Meteor Orbit Radar (CMOR) detected the shower using HF/VHF radar echos but the particles were too small for visual detection. Earth encountered the 1939 stream around 24 May 2019 8h UT with a ZHR of ~5. The Eta Aquariids also occur at this time of year. [19]
209P/LINEAR may also be the source of the weak 6–14 June meteor shower "sigma Ursae Majorids" (SIM #677). [11]
References
- ^ a b "IAUC 8314: P/2004 CB; 2004ba, 2004bb". IAU Central Bureau for Astronomical Telegrams. 2004-03-31. Retrieved 2012-10-03.
- ^ a b "209P/LINEAR Orbit". Minor Planet Center. Retrieved 2014-05-09.
- ^ a b c Syuichi Nakano (2011-10-31). "209P/LINEAR (NK 2142)". OAA Computing and Minor Planet Sections. Retrieved 2012-10-03.
- ^ "Horizons Batch for 209P/LINEAR on 2024-Jul-14" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Retrieved 2023-07-06. (JPL#141/Soln.date: 2023-Feb-13)
- ^ a b c "JPL Close-Approach Data: 209P/LINEAR" (last observation: 2014-05-26; arc: 10.48 years). Retrieved 2012-10-03.
- ^ a b c d Schleicher, David G.; knight, Matthew m. (27 September 2016). "The Extremely Low Activity Comet 209P/Linear During ITS Extraordinary Close Approach in 2014". The Astronomical Journal. 152 (4): 89. arXiv: 1605.01705. Bibcode: 2016AJ....152...89S. doi: 10.3847/0004-6256/152/4/89.
- ^ a b Howell, Ellen S.; Nolan, Michael C.; Taylor, Patrick A.; Springmann, Alessondra; Rodriguez-Ford, Linda; Zambrano-Marin, Luisa F.; Benner, Lance A.; Brozovic, Marina; Giorgini, Jon D.; Hergenrother, Carl (1 November 2014). "Radar images of Comet 209P/LINEAR: Constraints on shape and rotation". AAS/Division for Planetary Sciences Meeting Abstracts. 46: 209.24. Bibcode: 2014DPS....4620924H.
- ^ a b Gary W. Kronk. "209P/LINEAR". Cometography. Archived from the original on 2014-05-03. Retrieved 2014-05-03.
- ^ "IAUC 9005: COMET P/2008 X4 = P/2003 K2 (CHRISTENSEN); 208P; V5580 Sgr". IAU Central Bureau for Astronomical Telegrams. 2008-12-12. Retrieved 2012-10-03. (password required)
- ^ Alan Hale. "455. COMET 209P/LINEAR P/2008 X2". Earthrise Institute (Southwest Institute for Space Research). Retrieved 2012-10-03.
- ^ a b Peter Jenniskens. "May Camelopardalids". SETI Institute. Retrieved 2014-05-25.
- ^ a b "Arecibo Observatory Sees Comet 209P/LINEAR". Universities Space Research Association (USRA). 2014-05-29. Archived from the original on 2014-05-29. Retrieved 2014-05-29.
- ^ "Comets Waiting for First Observation". www.aerith.net.
- ^ a b c "The next big meteor shower". IMCCE. Archived from the original on 2012-10-06. Retrieved 2012-10-03.
- ^ "209P-ids 2014: prediction of activity". Archived from the original on 2014-04-14. Retrieved 2014-04-13.
- ^ a b Wiegert, Paul A.; Quanzhi Ye (2013). "Will Comet 209P/LINEAR Generate the Next Meteor Storm?". Monthly Notices of the Royal Astronomical Society. 437 (4): 3283–3287. arXiv: 1311.0235. Bibcode: 2014MNRAS.437.3283Y. doi: 10.1093/mnras/stt2127.
- ^ "Camelopardalids meteor shower a bust, but not a surprise". The Washington Post. 2014-05-24. 10:07AM. Retrieved 2014-05-24.
- ^ a b c "Camelopardalids 2014: First Results". International Meteor Organization. Archived from the original on 2014-05-25. Retrieved 2014-05-25.
- ^ "Meteor Activity Outlook for May 24–30, 2014". Archived from the original on 2014-05-25. Retrieved 2014-05-24.
External links
- Orbital simulation from JPL (Java) / Horizons Ephemeris
- 209P/LINEAR – Seiichi Yoshida @ aerith.net
- Elements and Ephemeris for 209P/LINEAR – Minor Planet Center
- 209P/LINEAR at the Minor Planet Center's Database
- 209P/LINEAR – Kazuo Kinoshita (Dec. 21, 2008 )
- Camelopardalids 2014: First Results
- May Camelopardalids ( SETI Institute / Peter Jenniskens)
- May Camelopardalids Fireball as seen from Pennsylvania via NASA Meteor Watch on Facebook
- How Scientists Chased a New Meteor Shower from the Sky (Space.com June 10, 2014)
- May Camelopardalids (MCM) May 24 2019 by CMOR radar
- Meteor activity related to 209P/LINEAR by worldwide radio meteor observations (2022)
.png)
|
| |
| Discovery | |
|---|---|
| Discovered by |
LINEAR 1.0-m reflector [1] |
| Discovery date | 3 February 2004 (asteroidal) 30 March 2004 (tail) |
| Designations | |
| 2004 CB | |
| Orbital characteristics | |
| Epoch | 2014-May-23 ( JD 2456800.5) [2] |
| Aphelion | 4.952 AU (Q) |
| Perihelion | 0.9695 AU (q) |
| Semi-major axis | 2.961 AU (a) |
| Eccentricity | 0.67258 |
| Orbital period | 5.09 yr |
| Inclination | 21.243° |
| Last perihelion | 2019-Jun-12
[2] 2014-May-06 [3] 2009-Apr-15 [3] |
| Next perihelion | 2024-Jul-14 [4] |
| Earth MOID | 0.05 AU (7,500,000 km) [5] |
| Physical characteristics | |
| Dimensions | 3.9 × 2.7 × 2.6 km [6] |
| 10.9 hours [7] | |
|
Comet total magnitude (M1) | 18.1 [5] |
209P/LINEAR is a periodic comet with an orbital period of 5.1 years. The comet has extremely low activity for its size and is probably in the process of evolving into an extinct comet. [6]
Observational history
The comet discovered on 3 February 2004 by Lincoln Near-Earth Asteroid Research (LINEAR) using a 1.0-metre (39 in) reflector. [1] Initially it was observed without a coma and named 2004 CB as a minor planet or asteroid, but in March 2004 Robert H. McNaught observed a comet tail which confirmed it as a comet. [8] It was given the permanent number 209P on 12 December 2008 as it was the second observed appearance of the comet. [9] Prediscovery images of the comet, dating back to December 2003, were found during 2009. [8]
209P/LINEAR came to perihelion (closest approach to the Sun) on 6 May 2014. [3] On 29 May 2014 the comet passed 0.0554 AU (8,290,000 km; 5,150,000 mi) from Earth, [5] but only brightened to about apparent magnitude 12. [10] The 2014 Earth approach was the 9th closest known comet approach to Earth. [11] The close approach allowed the comet nucleus to be imaged by Arecibo, producing the most detailed radar image of a comet nucleus to that date. [12] The radar imaging showed the comet nucleus is elongated and about 2.4 km by 3 km in size, [12] later refined to 3.9 × 2.7 × 2.6 km. [6] No evidence of large dust particles were detected in the coma. [7] The comet also had very low water production, (2.5±0.2)×1025 mol/s, from an active area measuring just 0.007 km². [6]
209P/LINEAR was recovered on 31 December 2018 at magnitude 19.2 by Hidetaka Sato. [13]
Associated meteor showers
Preliminary results by Esko Lyytinen and Peter Jenniskens, later confirmed by other researchers, predicted [14] [15] [16] 209P/LINEAR might a big meteor shower which would come from the constellation Camelopardalis on the night of 23/24 May 2014. It was possible that there could be 100 to 400 meteors per hour. [14] All the trails from the comet from 1803 through 1924 were expected to intersect Earth's orbit during May 2014. [14] The peak activity was expected to occur around 24 May 2014 7h UT when dust trails produced from past returns of the comet could pass 0.0002 AU (30,000 km; 19,000 mi) from Earth. [16] The 2014 Camelopardalids only generated 10–15 visual meteors per hour. [17] [18] But the expected radiant and date of visual maximum were correctly predicted. [18] The shower peaked around 6h UT on 24 May 2014. [18] The Canadian Meteor Orbit Radar (CMOR) detected the shower using HF/VHF radar echos but the particles were too small for visual detection. Earth encountered the 1939 stream around 24 May 2019 8h UT with a ZHR of ~5. The Eta Aquariids also occur at this time of year. [19]
209P/LINEAR may also be the source of the weak 6–14 June meteor shower "sigma Ursae Majorids" (SIM #677). [11]
References
- ^ a b "IAUC 8314: P/2004 CB; 2004ba, 2004bb". IAU Central Bureau for Astronomical Telegrams. 2004-03-31. Retrieved 2012-10-03.
- ^ a b "209P/LINEAR Orbit". Minor Planet Center. Retrieved 2014-05-09.
- ^ a b c Syuichi Nakano (2011-10-31). "209P/LINEAR (NK 2142)". OAA Computing and Minor Planet Sections. Retrieved 2012-10-03.
- ^ "Horizons Batch for 209P/LINEAR on 2024-Jul-14" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Retrieved 2023-07-06. (JPL#141/Soln.date: 2023-Feb-13)
- ^ a b c "JPL Close-Approach Data: 209P/LINEAR" (last observation: 2014-05-26; arc: 10.48 years). Retrieved 2012-10-03.
- ^ a b c d Schleicher, David G.; knight, Matthew m. (27 September 2016). "The Extremely Low Activity Comet 209P/Linear During ITS Extraordinary Close Approach in 2014". The Astronomical Journal. 152 (4): 89. arXiv: 1605.01705. Bibcode: 2016AJ....152...89S. doi: 10.3847/0004-6256/152/4/89.
- ^ a b Howell, Ellen S.; Nolan, Michael C.; Taylor, Patrick A.; Springmann, Alessondra; Rodriguez-Ford, Linda; Zambrano-Marin, Luisa F.; Benner, Lance A.; Brozovic, Marina; Giorgini, Jon D.; Hergenrother, Carl (1 November 2014). "Radar images of Comet 209P/LINEAR: Constraints on shape and rotation". AAS/Division for Planetary Sciences Meeting Abstracts. 46: 209.24. Bibcode: 2014DPS....4620924H.
- ^ a b Gary W. Kronk. "209P/LINEAR". Cometography. Archived from the original on 2014-05-03. Retrieved 2014-05-03.
- ^ "IAUC 9005: COMET P/2008 X4 = P/2003 K2 (CHRISTENSEN); 208P; V5580 Sgr". IAU Central Bureau for Astronomical Telegrams. 2008-12-12. Retrieved 2012-10-03. (password required)
- ^ Alan Hale. "455. COMET 209P/LINEAR P/2008 X2". Earthrise Institute (Southwest Institute for Space Research). Retrieved 2012-10-03.
- ^ a b Peter Jenniskens. "May Camelopardalids". SETI Institute. Retrieved 2014-05-25.
- ^ a b "Arecibo Observatory Sees Comet 209P/LINEAR". Universities Space Research Association (USRA). 2014-05-29. Archived from the original on 2014-05-29. Retrieved 2014-05-29.
- ^ "Comets Waiting for First Observation". www.aerith.net.
- ^ a b c "The next big meteor shower". IMCCE. Archived from the original on 2012-10-06. Retrieved 2012-10-03.
- ^ "209P-ids 2014: prediction of activity". Archived from the original on 2014-04-14. Retrieved 2014-04-13.
- ^ a b Wiegert, Paul A.; Quanzhi Ye (2013). "Will Comet 209P/LINEAR Generate the Next Meteor Storm?". Monthly Notices of the Royal Astronomical Society. 437 (4): 3283–3287. arXiv: 1311.0235. Bibcode: 2014MNRAS.437.3283Y. doi: 10.1093/mnras/stt2127.
- ^ "Camelopardalids meteor shower a bust, but not a surprise". The Washington Post. 2014-05-24. 10:07AM. Retrieved 2014-05-24.
- ^ a b c "Camelopardalids 2014: First Results". International Meteor Organization. Archived from the original on 2014-05-25. Retrieved 2014-05-25.
- ^ "Meteor Activity Outlook for May 24–30, 2014". Archived from the original on 2014-05-25. Retrieved 2014-05-24.
External links
- Orbital simulation from JPL (Java) / Horizons Ephemeris
- 209P/LINEAR – Seiichi Yoshida @ aerith.net
- Elements and Ephemeris for 209P/LINEAR – Minor Planet Center
- 209P/LINEAR at the Minor Planet Center's Database
- 209P/LINEAR – Kazuo Kinoshita (Dec. 21, 2008 )
- Camelopardalids 2014: First Results
- May Camelopardalids ( SETI Institute / Peter Jenniskens)
- May Camelopardalids Fireball as seen from Pennsylvania via NASA Meteor Watch on Facebook
- How Scientists Chased a New Meteor Shower from the Sky (Space.com June 10, 2014)
- May Camelopardalids (MCM) May 24 2019 by CMOR radar
- Meteor activity related to 209P/LINEAR by worldwide radio meteor observations (2022)
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