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Search references for PALMER DIVIDE. Phrases containing PALMER DIVIDE
See searches and references containing PALMER DIVIDE!PALMER DIVIDE
Ridge in Colorado, United States
The Palmer Divide is a caprock escarpment-style ridge in central Colorado that separates the Arkansas River basin from the South Platte basin. It extends
Palmer_Divide
Town in Colorado, United States
of it (0.65%) is water. The town marks the top of the Palmer Divide, a ridge running from Palmer Lake eastward which separates the Arkansas River drainage
Palmer_Lake,_Colorado
Asteroid
2004, the first lightcurve by American astronomer Brian Warner at his Palmer Divide Observatory (PDS) in Colorado, gave a rotation period of 5.487 hours
2001_Einstein
Mountain pass in Colorado, USA
Forest Divide Pass is a 7,352 feet (2,241 m) elevation mountain pass in the Palmer Divide in central Colorado in the United States. The pass dividing the
Monument_Hill_(Colorado)
Region of Colorado, US
Gleneagle, King's Deer, and Black Forest. The region lies along the Palmer Divide about 40 miles (64 kilometers) south of Denver and 20 miles (32 kilometers)
Tri-Lakes,_Colorado
Archaeological site in Colorado, United States
of Denver on the north edge of the Palmer Divide. It is the largest rock shelter documented on the Palmer Divide, which contains artifacts from many
Franktown_Cave
Asteroid orbiting the Sun
Massachusetts, in the USA. Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado in 2007 gave a light curve
747_Winchester
Main-belt asteroid
In 2009, Photometric observations of this asteroid were made at the Palmer Divide Observatory in Colorado Springs, Colorado. The resulting asymmetrical
118_Peitho
Main-belt asteroid
and a brightness variation of 0.35 in magnitude. A 2008 study at the Palmer Divide Observatory in Colorado Springs, Colorado gave a period of 11.309 ±
176_Iduna
Main-belt asteroid
meteorite, although with a higher albedo. Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado during 2007 produced a light
92_Undina
Topics referred to by the same term
community Palmer Creek (Turnagain Arm), Alaska Palmer Creek (Yamhill River), Oregon Palmer Divide, Colorado, a ridge Palmer Glacier, Oregon Palmer Park (Chicago)
Palmer
Carbonaceous main-belt asteroid
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a well-defined rotation
1930_Lucifer
Hungaria asteroid
photometric observations by American astronomers Brian Warner at his Palmer Divide Observatory, Colorado, and Robert Stephens at the Center for Solar System
5806_Archieroy
Asteroid orbiting the Sun in the main belt of asteroids
March 1888 in Vienna. Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado, in 2007 gave a light curve
273_Atropos
Asteroid in the main belt of asteroids
In 2009, photometric observations of this asteroid were made at the Palmer Divide Observatory in Colorado Springs, Colorado. The resulting light curve
193_Ambrosia
Hungaria asteroid and a suspected contact-binary
Magoeba were obtained by American astronomer Brian Warner at the CS3–Palmer Divide Station (U82) in California. Lightcurve analysis of the photometric
1355_Magoeba
Carbonaceous asteroid of the Apollo group
photometric observations made by American astronomer Brian Warner at his Palmer Divide Observatory, Colorado, in February 2015. The ambiguous lightcurve rendered
(416151)_2002_RQ25
Main-belt asteroid
of the astronomer Camille Flammarion. Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado in during 2007 produced a
154_Bertha
Hungaria asteroid and suspected binary system
Warner, Brian D. (January 2009). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 May - September". The Minor Planet Bulletin. 36 (1):
4868_Knushevia
Main-belt asteroid
studied by radar. Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado in 2007 gave a light curve
28_Bellona
S-type Main-belt asteroid
S-type asteroid based on its spectrum. Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado during 2007 produced a light
170_Maria
American astronomer (b. 1952)
operated from the Palmer Divide Observatory at his home near Colorado Springs, Colorado. Since 2011 he has operated from the Palmer Divide Station (U82) at
Brian_D._Warner
Main-belt asteroid
probably composed of carbonaceous material. Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado, during 2007 produced a light
275_Sapientia
Asteroid
photometric observations by American astronomer Brian Warner at his Palmer Divide Station in Colorado. It gave a well-defined rotation period of 1320±10
9165_Raup
Mars-crossing asteroid
lightcurve was obtained from photometric observations by Brian Warner at the Palmer Divide Station in Colorado. Lightcurve analysis gave a rotation period of 460±5
6141_Durda
Main-belt asteroid
varied in brightness. Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado, during 2007–8 gave a light
167_Urda
Carbonaceous background asteroid
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory (716) in Colorado. Lightcurve analysis gave a longer-than
1092_Lilium
American engineer and veteran of the Civil War (1836–1909)
needed] Palmer Divide, a geographic feature north of Colorado Springs, and the community of Palmer Lake, Colorado, are named after him, as is Palmer Park
William_Jackson_Palmer
Main-belt asteroid
diameter. Photometric observations by astronomer Brian D. Warner at the Palmer Divide Observatory in Colorado (716) during winter 2007–2008 were used to build
2093_Genichesk
Minor planet orbiting the Sun
Monterosa is a minor planet orbiting the Sun. Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado during 2007 produced a light
947_Monterosa
Main-belt asteroid
183–185, Bibcode:2011MPBu...38..183P. Lightcurve plot of 224 Oceana, Palmer Divide Observatory, B. D. Warner (2006) Asteroid Lightcurve Database (LCDB)
224_Oceana
Main-belt asteroid
of 0.30 in magnitude (U=2-). American astronomer Brian Warner at the Palmer Divide Observatory (716), Colorado, originally took the photometric observations
1329_Eliane
Asteroid
photometric lightcurve analysis by U.S. astronomer Brian Warner at his Palmer Divide Observatory (716), Colorado, gave a well-defined rotation period of
3728_IRAS
Mars-crossing asteroid
Karayusuf was obtained from photometric observations by Brian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a well-defined rotation
3800_Karayusuf
Main-belt asteroid
Binary Discoveries From The Palmer Divide Observatory, Brian Warner (2014) Lightcurve plot of 4383 Suruga, Palmer Divide Observatory, B. D. Warner (2013)
4383_Suruga
Mars-crossing asteroid
December 2016. The Palmer Divide Observatory: Tour given by Brian Warner on YouTube (time 4:03 min.) Lightcurve plot of 2449 Kenos, Palmer Divide Observatory
2449_Kenos
Main-belt Flora asteroid
lightcurve analysis of Modra by American astronomer Brian Warner at his Palmer Divide Observatory, Colorado, rendered an unambiguous period of 27.12±0.02
11118_Modra
Minor planet orbiting the Sun
Raphaela is a minor planet orbiting the Sun. Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado during 2007 produced a light
708_Raphaela
Main-belt asteroid
17 October 2019. Warner, B. (June 2001). "Asteroid Photometry at the Palmer Divide Observatory". The Minor Planet Bulletin. 28: 30–32. Bibcode:2001MPBu
1659_Punkaharju
Asteroid on an eccentric orbit
photometric observations by American astronomer Brian Warner at the Palmer Divide Station (U82) in California. Lightcurve analysis gave a consolidated
(90075)_2002_VU94
Main-belt asteroid
and a brightness variation of 0.32 in magnitude. A 2007 study at the Palmer Divide Observatory in Colorado, United States, yielded a period of 20.666 ±
148_Gallia
Asteroid
Warner, Brian D. (July 2009). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 December - 2009 March". The Minor Planet Bulletin
1656_Suomi
Dark asteroid
Warner, Brian D. (October 2010). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2010 March - June" (PDF). Minor Planet Bulletin. 37 (4):
2204_Lyyli
Very large asteroid in the main belt of asteroids
carbonaceous material. Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado, during 2007 gave a light
365_Corduba
Flora family asteroid
of Annette was obtained by American astronomer Brian Warner at his Palmer Divide Observatory, Colorado, in December 2005. It gave a rotation period of
2839_Annette
Asteroid
photometric observations by American astronomer Brian Warner at this Palmer Divide Observatory in Colorado. Lightcurve analysis gave a well-defined rotation
4217_Engelhardt
Probable rare-type binary asteroid
lightcurve was obtained by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a rotation period
(5646)_1990_TR
Main-belt asteroid
Pamela was obtained from photometric observations by Brian Warner at his Palmer Divide Observatory in Colorado, United States. Lightcurve analysis gave a rotation
1243_Pamela
Main-belt asteroid
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a well-define rotation
1307_Cimmeria
Minor planet (asteroid) orbiting in the Asteroid Belt
friend of the astronomer. Photometric observations of this asteroid at Palmer Divide Observatory in Colorado Springs, Colorado during 2007 gave a light curve
607_Jenny
Minor planet (asteroid)
Koran name for the Queen of Sheba. Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado in 2006–7 were used to build
585_Bilkis
Asteroid
Wallonia was obtained from photometric observations by Brian Warner at the Palmer Divide Observatory in Colorado, United States. Lightcurve analysis gave a rotation
3198_Wallonia
Main-belt asteroid
taxonomy system lists it as an Sw asteroid. Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado in during 2007 produced a
108_Hecuba
Main-belt asteroid
In 2009, Photometric observations of this asteroid were made at the Palmer Divide Observatory in Colorado Springs, Colorado. The resulting light curve
191_Kolga
Dark background asteroid
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory (716) in Colorado. Lightcurve analysis gave two divergent
1266_Tone
Main Belt Asteroid
asteroid's provisional designation 1905 RE. Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado in 1999 were used to build
575_Renate
Main-belt asteroid binary
rotational lightcurves of Jedicke from photometric observations at his Palmer Divide Station in Colorado, United States. Best rated lightcurve analysis from
5899_Jedicke
Asteroid
photometric observations made American astronomer by Brian Warner at his Palmer Divide Observatory in Colorado. The lightcurve gave a rotation period of 5
7816_Hanoi
Mars-crossing asteroid
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory (716) in Colorado. Lightcurve analysis gave a rotation period
3635_Kreutz
Main-belt asteroid
diameter. Photometric measurements of the asteroid made in 2005 at the Palmer Divide Observatory showed a light curve with a period of 2.572 ± 0.002 hours
2131_Mayall
Asteroid
previous 2006-observation by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado gave a period of 6.510 hours and an amplitude
(7563)_1988_BC
Large and dark background asteroid
hours and amplitude of at least 0.11 magnitude by Brian Warner at his Palmer Divide Observatory in Colorado from November 1999 (U=2). In 2006, Warner revised
868_Lova
Asteroid
coordinates. Summary figures at the LCDB Lightcurve plot of 1103 Sequoia, Palmer Divide Observatory, B. D. Warner (2011). Summary figures at the LCDB "JPL Small-Body
1103_Sequoia
Stony Hungaria asteroid and Mars-grazer
Nemrut Dagi was obtained by American astronomer Brian Warner at his CS3–Palmer Divide Station (U82) in California. Lightcurve analysis gave a well-defined
20936_Nemrut_Dagi
Main-belt asteroid
(help) The Palmer Divide Observatory: Tour given by Brian Warner on YouTube (time 4:03 min.) Lightcurve plot of 1207 Ostenia, Palmer Divide Observatory
1207_Ostenia
Asteroid
photometric observations made by American astronomer Brian Warner at his Palmer Divide Observatory (716) in September 2003. The revised lightcurve showed a
4209_Briggs
Hungaria asteroid and slow rotator
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory (716) in Colorado. It gave a long rotation period of 105
3043_San_Diego
Asteroid
of 0.12 magnitude was measured by photometrist Brian Warner at his Palmer Divide Observatory in Colorado, United States (U=3-). According to the surveys
1015_Christa
Minor planet orbiting the Sun
Analysis at the Palmer Divide Observatory", The Minor Planet Bulletin, Bibcode:2007MPBu...34...72W. Lightcurve plot of 572 Rebekka, Palmer Divide Observatory
572_Rebekka
Dark background asteroid from the central regions of the asteroid belt
Massachusetts during January 2006, by American Brian Warner at the Palmer Divide Observatory (716) in Colorado Springs, Colorado, were used to generate
4547_Massachusetts
Eccentric, stony asteroid
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory, Colorado, in August 2014 and March 2015, respectively.
4401_Aditi
Large, dark, P-type main-belt asteroid
studied by radar. Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado in 2007 gave a light curve
56_Melete
Main-belt asteroid
photometric observation of the asteroid's light-curve performed at the Palmer Divide Observatory during 1999 rendered a rotation period of 5.892±0.002 hours
771_Libera
Carbonaceous-dark main-belt asteroid
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a longer-than average
1952_Hesburgh
Main-belt asteroid
08.016 The Palmer Divide Observatory: Tour given by Brian Warner on YouTube (time 4:03 min.) Lightcurve plot of 1222 Tina, Palmer Divide Observatory
1222_Tina
Stony main-belt asteroid
photometric observations by American astronomer Brian D. Warner at his Palmer Divide Observatory in Colorado. It gave a rotation period of 8.481 hours with
1817_Katanga
Asteroid
have been named for Drake University. Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado, in 2001 were used to build
620_Drakonia
Near-Earth asteroid
Warner, Brian D. (January 2013). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2012 June - September" (PDF). Minor Planet Bulletin. 40
1685_Toro
Main-belt asteroid
6 km. Photometric measurements of the asteroid made in 2005 at the Palmer Divide Observatory showed a light curve with a rotation period of 6.87±0.01 h
400_Ducrosa
Asteroid
photometric observations by American astronomer Brian Warner at the CS3–Palmer Divide Station in California (U82). Lightcurve analysis gave a rotation period
(85713)_1998_SS49
Hungaria asteroid and suspected tumbler
lightcurve was obtained by American astronomer Brian Warner at his Palmer Divide Observatory (716) in Colorado. Lightcurve analysis gave a rotation period
1919_Clemence
Main-belt asteroid
photometric observations made by American astronomer Brian Warner at the U.S. Palmer Divide Observatory, Colorado, in July 2013. It gave a rotation period of 3
7959_Alysecherri
Hungaria asteroid
photometric observations made by American astronomer Brian Warner at his Palmer Divide Observatory (716) between 2008 and 2016. They all gave a concurring
4031_Mueller
Minor planet (asteroid) orbiting in the asteroid belt
1905 from Heidelberg. Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado, during 2008 gave a light
568_Cheruskia
Main-belt asteroid
measurements show a large diameter of 179 km. Photometric observations at the Palmer Divide Observatory during 2005 showed a rotation period of 5.7366±0.0005 hours
209_Dido
Hungaria asteroid
lightcurves for this asteroid from photometric observations at the CS3–Palmer Divide Station in Colorado. The lightcurves gave a well-defined rotation period
(6382)_1988_EL
Hungaria asteroid
Planets in 1955 (H 97). Lightcurve plot of (1019) Strackea, Warner (2014) Palmer Divide Station. Summary figures at Center for Solar System Studies "JPL Small-Body
1019_Strackea
Hungaria asteroid
Brian D. Warner obtained another 3 well-defined lightcurves at the U.S. Palmer Divide Station, Colorado. They gave a slightly longer period of 5.193–5.203
4713_Steel
Hungaria asteroid, suspected binary system and asteroid pair
obtained from photometric observations by astronomers Brian Warner at his Palmer Divide Observatory (716), Petr Pravec at Ondřejov Observatory, and Julian Oey
4765_Wasserburg
Main-belt asteroid
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a rotation period
24827_Maryphil
Minor planet that orbits in the asteroid belt
Camille Flammarion had his observatory. Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado, in 1999 were used to build
605_Juvisia
Sub-kilometer asteroid
photometric observations by American astronomer Brian Warner at the CS3–Palmer Divide Station (U82) in Landers, California. It gave a longer-than average
(374158)_2004_UL
Asteroid
(U=3). Previously in June 1999, observations by Brian Warner at his Palmer Divide Observatory (716) in Colorado only gave a period of above 24 hours and
898_Hildegard
Hungaria asteroid and a possible binary system
photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a well-defined rotation
4440_Tchantchès
Main-belt asteroid
15.8° to the plane of the ecliptic. Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado during the winter of 2007–2008
793_Arizona
Minor planet orbiting in the asteroid belt
asteroid's provisional designation 1905 RC. Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado from 2001 to 2006 were used
573_Recha
Main-belt asteroid
object is now known as 1317 Silvretta. Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado in 1999 were used to build
787_Moskva
Mars-crossing asteroid
photometric observations by American photometrist Brian Warner at the Palmer Divide Observatory in Colorado. Lightcurve analysis gave a rotation period
4142_Dersu-Uzala
Asteroid
the preliminary designation 1909 HG. Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado, in 1999 were used to build
687_Tinette
Main-belt asteroid
observations of Luu collected by American astronomer Brian D. Warner at his Palmer Divide Station, Colorado, show a rotation period of 13.55±0.02 hours with a
5430_Luu
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