The Asteroid/Comet Connection's daily news journal about asteroids, comets, and meteors Today's issue status: done
Cover: As 2004 FY31 raced from its discovery location (discovered by LONEOS March 31.30, upper-right red dot), Peter Birtwhistle in England pursued it through Draco and into Cygnus and the Milky Way (images and orange dots), where the last optical observation came from Tenagra II Observatory on April 11.47 after passing Earth at 12.1 lunar distances on the 10th. Arecibo radar caught it on April 14.54 (lower-left red dot). See Great Shefford Observatory's 2004 FY31 page for further explanation, an animation, and a different star chart. At JPL's absolute magnitude H=21.89 calculation, FY31 is bright enough to squeak into the potentially hazardous category. |
| Small objects – panel 1/2 | Major News for 18 April 2004 |
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Small objects It was another spectacular week for small objects, those with absolute magnitude calculated at greater than H=22.0, which converts to roughly smaller than 135 meters/yards wide. Nine discoveries were announced, and the smallest actually flew through the Earth-Moon system early today UT. That one, 2004 HE, was discovered by Michael Van Ness at LONEOS, while the other eight were found by LINEAR. Besides the discoveries, another eight small objects were tracked, and older observations were reported for seven more. All this work was done by some 38 professional, educational, and amateur observing facilities plus one archive sleuth, but, oddly enough, neither of the Spacewatch telescopes were involved. Of special note this week is the work of amateur astronomer Krisztian Sarneczky of the Szeged University (SZTE) Asteroid program in Hungary. Among his new data reported last week from the NEAT archives were observations that extended the old observing arcs of four small objects and added |
positions for two more (and also updated a larger object on April 14th that has impact solutions). Early today UT, 2004 HE was at 0.72 lunar distance (LD). Checking the Sormano SAEL and JPL Close Approaches for other flybys, 2004 HM was at 5.1 LD last Tuesday, and 2004 HL was at 5.6 LD and 2004 GD2 at 9.6 LD on Wednesday. This coming week, 2004 GD will be at 6.0 LD on Tuesday and 2004 HB at 10.2 LD on Wednesday. << previous report | skip table | Small objects table >>
If an asteroid's orbit brings it to within 0.05 AU of Earth's orbit, it is categorized as "potentially hazardous" unless it has an absolute magnitude H greater than 22.0, which corresponds to a diameter on the order of 135
Notes: Diameters in the following table are rough best estimates from a very inexact H-to-size formula using H (absolute magnitude) from the JPL NEO Orbital Elements page, source also for Earth MOID (minimum orbital intersection). Other MOIDs are from Lowell Observatory. Current MPC H is also given, along with discovery MPEC H. Priorities and visibilities are from the European Spaceguard Central Node (SCN). |
| Small objects – panel 2/2 (table) | Major News for 18 April 2004 |
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H = absolute magnitude (brightness), from which size is roughly estimated — m/yd = meters/yards — [cross index]
All objects had observations reported last week. Those on a light-blue background had observations from only before the week.
Object | Estimated diameter | JPL H | MPC H | Discovery H in MPEC |
Earth MOID | European Spaceguard Central Node priority/visibility/campaign |
|---|---|---|---|---|---|---|
| 2004 HE Apollo | 15 m/yd | 26.75 | 26.7 | 26.7 2004-H16 | 0.00004 AU | |
| NEW: 2004 HE was discovered on 16 April by LONEOS, was confirmed on 16 April by the Siding Spring Survey (SSS) and KLENOT, and on 17 April by Robert Hutsebaut via New Mexico Skies (see yesterday's cover), Mt. John Obs., and SSS, and was announced in MPEC 2004-H16 yesterday. No observations were reported today. It has an MOID of 0.027 AU with Mars, and early today passed the Earth at 0.722 LD and then the Moon at 0.639 LD. See yesterday's special report. | ||||||
| 2004 FM32 Apollo | 16 m/yd | 26.59 | 27.1 | 27.2 2004-G01 | 0.00221 AU | Necessary, visibility ends 22 Apr. |
| 2004 FM32 was observed on 14 April by Tim Spahr from Whipple Obs. | ||||||
| 2004 FH Aten | 18 m/yd | 26.42 | 25.7 | 25.7 2004-F24 | 0.00008 AU | |
| 2004 FH was reported this last week as observed on 18 March by Bisei Spaceguard Center (BSC). It has an MOID of 0.009 AU with Venus. | ||||||
| 2004 HL Apollo | 18 m/yd | 26.41 | 26.5 2004-H24 | 0.01407 AU | ||
| NEW: 2004 HL was discovered on 16 April by LINEAR, was confirmed on 17 April by LINEAR and Mt. John Obs., and was announced in MPEC 2004-H24 of 18 April. It passed Earth at 5.6 LD on April 14th. | ||||||
| 2004 HD Amor | 42 m/yd | 24.53 | 24.5 | 24.5 2004-H19 | 0.03049 AU | |
| NEW: 2004 HD was discovered on 16 April by LINEAR, was confirmed on 16 April by Andrushivka Obs. and KLENOT, and on 17 April by Southern TIE (SoTIE), Tenagra II Obs., and Powell Obs., and was announced in MPEC 2004-H19 yesterday. Update MPEC 2004-H23 today reports that this object was also observed on 16 April by LINEAR, Andrushivka Obs., and KLENOT and on 17 April by SoTIE, Tenagra II Obs., Powell Obs., Sabino Canyon Obs., and SSS. It will pass the Earth at 13.7 LD on April 20th. | ||||||
| 2004 GD2 Apollo | 51 m/yd | 24.12 | 24.3 | 24.2 2004-G28 | 0.01999 AU | Necessary, visibility ends 7 Jun. |
| NEW: 2004 GD2 was discovered on 12 April by LINEAR, was confirmed on 12 April by Obs. Astronomico de Mallorca (OAM) and Consell Obs., and on 13 April by Andrushivka Obs., Sabino Canyon Obs., Table Mountain Obs., Tenagra II Obs., Desert Moon Obs., and Hutsebaut/NM Skies (see Tuesday's cover), and was announced in MPEC 2004-G28 of 13 April. This object was also observed on 13 April by LINEAR, Great Shefford Obs., OAM, and Golden Hill Obs., on 14 April by Great Shefford Obs., Hobbs Obs., Powell Obs., OAM, LINEAR, and Buchloe Obs., on 15 April by LINEAR, and on 16 April by LINEAR. It has an MOID of 0.001 AU with Mars, and passed Earth at 9.6 LD on April 14th. | ||||||
| 1996 TD9 Apollo | 51 m/yd | 24.10 | 24.0 1996-T07 | 0.02220 AU | ||
| 1996 TD9 was reported this week as found by Krisztian Sarneczky in 18 Oct. 1996 NEAT/Haleakala archives. This added three positions and 1.727 days to what had been a 4.099-day observing arc with 23 observations. | ||||||
| 2004 GC19 Apollo | 53 m/yd | 24.04 | 24.1 | 24.1 2004-H06 | 0.03498 AU | Urgent, visibility ends 28 Apr. |
| NEW: 2004 GC19 was discovered on 15 April by LINEAR, was confirmed on 15 April by Great Shefford Obs., and on 16 April by Andrushivka Obs., Sabino Canyon Obs., Tenagra II Obs., and Hutsebaut/NM Skies, and was announced in MPEC 2004-H06 of 16 April. This object was also observed on 16 April by LINEAR and Hutsebaut/NM Skies. | ||||||
| 2004 GZ14 Apollo | 53 m/yd | 24.02 | 24.0 | 24.0 2004-G44 | 0.02769 AU | Necessary, visibility ends 29 Apr. |
| NEW: 2004 GZ14 was discovered on 14 April by LINEAR, was confirmed on 14 April by Great Shefford Obs., Drebach Obs., Starkenburg Obs., Ondrejov Obs., and KLENOT, and on 15 April by Modra Obs., Sabino Canyon Obs., Tenagra II Obs., and Desert Moon Obs., and was announced in MPEC 2004-G44 of 15 April. This object was also observed on 15 April by LINEAR and on 17 April by Linz Obs. | ||||||
| 2004 EU22 Apollo | 62 m/yd | 23.68 | 23.7 | 23.7 2004-F22 | 0.00801 AU | Useful, visibility ends 25 May |
| 2004 EU22 was observed on 18 March by BSC, on 11 April by Sandlot Obs., on 12 April by LINEAR, on 14 April by Powell Obs., and on 15 April by Wildberg Obs. and Petit Jean Mountain Obs. | ||||||
| 2004 GD Apollo | 63 m/yd | 23.65 | 23.7 | 23.8 2004-G17 | 0.00600 AU | Urgent, visibility ends 23 Apr. |
| 2004 GD was observed on 11 April by Guidestar Obs., on 12 April by Guidestar Obs., on 13 April with the Australian Natl. Univ. (ANU) Obs. 1.0m telescope, on 14 April by Great Shefford Obs., Buchloe Obs., and Uccle Obs., on 15 April by Great Shefford Obs., and on 16 April by Goodricke-Pigott Obs. It has an MOID of 0.033 AU with Venus, and will pass the Earth at 6.0 LD on April 20th. | ||||||
| 2004 FB18 Amor | 64 m/yd | 23.61 | 23.9 | 23.5 2004-F76 | 0.05857 AU | Useful, visibility ends 15 Jun. |
| 2004 FB18 was observed on 11 April by Tenagra II Obs. and on 14 April by Tim Spahr from Whipple Obs. | ||||||
| 2004 HB Apollo | 72 m/yd | 23.36 | 23.3 | 23.3 2004-H17 | 0.02128 AU | |
| NEW: 2004 HB was discovered on 16 April by LINEAR, was confirmed on 16 April by KLENOT, and on 17 April by SoTIE and Tenagra II Obs., and was announced in MPEC 2004-H17 of 17 April. This object was also observed on 17 April by LINEAR. It will pass Earth at 10.2 LD on April 21st. | ||||||
| 2001 TE45 Apollo | 78 m/yd | 23.18 | 23.3 2001-U13 | 0.09458 AU | ||
| 2001 TE45 was reported this as found by Sarneczky in 16 and 20 Oct. 2001 NEAT/Palomar archives. This added five positions inside the existing observing arc that previously had had only 20 observations. | ||||||
| 2004 HM Apollo has impact solutions | 88 m/yd | 22.92 | 23.3 2004-H25 | 0.00338 AU | ||
| NEW: 2004 HM was discovered on 16 April by LINEAR, was confirmed on 17 April by LINEAR, Tenagra II Obs., and Mt. John Obs., and on 18 April by Pla D'Arguines Obs., OAM, Sabino Canyon Obs., and Tenagra II Obs., and was announced in MPEC 2004-H25 today. It passed Earth at 5.1 LD on April 13th. | ||||||
| 2004 FP4 Amor | 89 m/yd | 22.91 | 23.2 | 23.3 2004-F47 | 0.05278 AU | Useful, visibility ends 22 Jul. |
| 2004 FP4 was observed on 9 April by Mt. John Obs., on 12 April by LONEOS, on 13 April by Tenagra II Obs., and on 17 April by LINEAR. It has an MOID of 0.009 AU with Mars. | ||||||
| 2004 GB19 Apollo | 100 m/yd | 22.64 | 22.7 | 22.7 2004-H04 | 0.01053 AU | Urgent, visibility ends 25 May |
| NEW: 2004 GB19 was discovered on 15 April by LINEAR, was confirmed on 15 April by Great Shefford Obs., and on 16 April by Andrushivka Obs., Sabino Canyon Obs., and Hutsebaut/NM Skies, and was announced in MPEC 2004-H04 of 16 April. This object was also observed on 16 April by LINEAR. It has an MOID of 0.011 AU with Mars. | ||||||
| 2001 UF5 Apollo | 110 m/yd | 22.44 | 22.9 | 22.2 2001-U38 | 0.00581 AU | |
| 2001 UF5 was reported by Sarneczky from archives as observed on 20 Oct. 2001 by NEAT/Haleakala and NEAT/Palomar. This added seven positions early within the existing observation arc that previously had had only 32 observations. 2001 UF5 has MOIDs of 0.000 AU with Venus and 0.001 AU with Mars. | ||||||
| 2001 SQ263 Aten | 112 m/yd | 22.41 | 22.6 | 22.4 2001-S50 | 0.03203 AU | |
| 2001 SQ263 was reported by Sarneczky from archives as observed on 30 Sept. and 6 and 13 Oct. 2001 by NEAT/Palomar. This added eight positions and 1.969 days to what had been an 17.973-day observing arc with 30 observations. 2001 SQ263 has MOIDs of 0.028 AU with Mercury and 0.031 AU with Venus. | ||||||
| 2001 UE18 Amor | 119 m/yd | 22.27 | 22.5 | 22.1 2001-U69 | 0.19148 AU | |
| 2001 UE18 was reported by Sarneczky from archives as observed 27 and 29 Oct. 2001 by NEAT/Palomar. This added six positions and 1.007 days to what had been a 1.945-day arc with nine observations. | ||||||
| 2002 FT6 Aten | 120 m/yd | 22.26 | 22.5 | 22.7 2002-F73 | 0.04082 AU | |
| 2002 FT6 was observed 15 April by Carl Hergenrother from Whipple Obs., following up on the recovery A/CC reported April 5th | ||||||
| 1997 VG Amor | 121 m/yd | 22.24 | 22.5 1997-V06 | 0.08077 AU | ||
| 1997 VG was reported by Sarneczky from archives as observed 30 Oct. 1997 by NEAT/Haleakala. This added 1.759 days to what had been an 8.078-day observing arc. | ||||||
| 2004 BW18 Amor | 124 m/yd | 22.18 | 22.6 | 22.5 2004-B24 | 0.04478 AU | Useful, visibility ends 30 May |
| 2004 BW18 was observed on 13 April by Hunters Hill Obs. | ||||||
| 2004 EO20 Amor | 131 m/yd | 22.06 | 22.2 | 21.6 2004-F14 | 0.16088 AU | Useful, visibility ends 25 May |
| 2004 EO20 was observed on 14 April by Tim Spahr from Whipple Obs. | ||||||
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| News briefs – panel 1/1 | Major News for 18 April 2004 |
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News briefs
Comet news: After an interruption earlier today, SOHO images of C/2004 F4 (Bradfield)'s perihelion passage have resumed being posted from intervals that are almost hourly. You can watch the spectacular show from here or here. MPEC 2004-H26 today announces the newest comet discovery, C/2004 H1 (LINEAR). From the first very preliminary calculation, it reached perihelion this last January 13th out past Mars on a retrograde path (i=141.2°) — "driving on the wrong side of the Solar System," one might say. The first LINEAR observation in the MPEC is from early Friday, and it and four other observing facilities confirmed the object yesterday and today. |
Namings: The Minor Planet Center updated its Discovery Circumstances page April 16th with 65 new names, all for asteroids discovered by the LINEAR program, and all named for high school student finalists and finalist mentors in the 2004 Intel Science Talent Search (STS). You can read about them at LINEAR's Ceres Connection Winners for 2004 page, and in the STS 2004 finalists list. They include Lisa Glukhovsky, whose project was "A Rapid, Accurate Method of Determining the Distance to Near-Earth Asteroids." And, nothing to do with astronomy or even gastronomy, but, rather, biochemistry, we have to also mention Jennifer D'Ascoli, whose project was blueberry pie. The last MPC namings update was March 5th. |
| Risk monitoring - panel 1/1 | Major News for 18 April 2004 |
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JPL has posted 2004 HM, which was announced today in MPEC 2004-H25 as discovered early Friday by LINEAR in New Mexico, which also caught it yesterday morning, followed by Tenagra II Observatory in Arizona and then Mt. John Observatory in New Zealand. The confirmation process was closed out this morning by Pla D'Arguines Observatory in Spain and the Observatorio Astronomico de Mallorca (OAM), followed by Sabino Canyon and Tenagra II observatories in Arizona. JPL puts 2004 HM's diameter at about 90 meters/yards. The Sunday Daily Orbit Update MPEC has observation of 2004 GE2 from LINEAR in New Mexico yesterday morning. Today JPL cut its impact solution count from five to one (in the year 2100) and slightly lowered its overall risk ratings for this object. |
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