Loading…
Astrometric Observations of the Galilean Moons of Jupiter at the Pulkovo Normal Astrograph in 2016−2017
We present the results of observations of the Galilean moons of Jupiter carried out at the Normal Astrograph of the Pulkovo Observatory in 2016−2017. We obtained 761 positions of the Galilean moons of Jupiter in the system of the Gaia DR1 catalog (ICRF, J2000.0) and 854 differential coordinates of t...
Saved in:
| Published in: | Solar system research 2018-07, Vol.52 (4), p.312-319 |
|---|---|
| Main Authors: | , , , , , , , , |
| Format: | Article |
| Language: | English |
| Subjects: | |
| Citations: | Items that this one cites Items that cite this one |
| Online Access: | Get full text |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| cited_by | cdi_FETCH-LOGICAL-c316t-a115f33b37e06e2c2ce48006df07a5a084ee0fb6f78a1744f033900d4ca52bf33 |
|---|---|
| cites | cdi_FETCH-LOGICAL-c316t-a115f33b37e06e2c2ce48006df07a5a084ee0fb6f78a1744f033900d4ca52bf33 |
| container_end_page | 319 |
| container_issue | 4 |
| container_start_page | 312 |
| container_title | Solar system research |
| container_volume | 52 |
| creator | Narizhnaya, N. V. Khovrichev, M. Yu Apetyan, A. A. Bikulova, D. A. Ershova, A. P. Balyaev, I. A. Kulikova, A. M. Os’kina, K. I. Maksimova, L. A. |
| description | We present the results of observations of the Galilean moons of Jupiter carried out at the Normal Astrograph of the Pulkovo Observatory in 2016−2017. We obtained 761 positions of the Galilean moons of Jupiter in the system of the Gaia DR1 catalog (ICRF, J2000.0) and 854 differential coordinates of the satellites relative to each other. The mean errors in the satellites’ normal places and the corresponding root-mean-square deviations are ε
α
= 0.0020′′, ε
δ
= 0.0027′′, σ
α
= 0.0546′′, and σ
δ
= 0.0757′′. The equatorial coordinates of the moons are compared to the motion theories of planets and satellites. On average, the (O–C) residuals in the both coordinates relative to the motion theories are less than 0.031′′. The best agreement with observations is achieved by a combination of the EPM2015 and V. Lainey-V.2.0|V1.1 motion theories, which yields the average (O–C) residuals of approximately 0.02″. Peculiarities in the behavior of the (O–C) residuals and error values in Ganymede have been noticed. |
| doi_str_mv | 10.1134/S0038094618040020 |
| format | article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2071143691</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2071143691</sourcerecordid><originalsourceid>FETCH-LOGICAL-c316t-a115f33b37e06e2c2ce48006df07a5a084ee0fb6f78a1744f033900d4ca52bf33</originalsourceid><addsrcrecordid>eNp1kMFOwzAQRC0EEqXwAdwscQ7s2q6THqsKCqhQJOAcOandpqRxsJ1K_AFnPpEvIWkrcUCcRtp5MysNIecIl4hcXD0D8ASGQmICAoDBAemhhCTigvFD0uvsqPOPyYn3KwAEiGWPFCMfnF3r4IqczjKv3UaFwlaeWkPDUtOJKotSq4o-2P31vqmLoB1VYQs8NeWb3Vj6aN1alXTbt3CqXtKiogxQfn9-tRKfkiOjSq_P9tonrzfXL-PbaDqb3I1H0yjnKEOkEAeG84zHGqRmOcu1SADk3ECsBgoSoTWYTJo4URgLYYDzIcBc5GrAsjbZJxe73trZ90b7kK5s46r2ZcogRhRcDrGlcEflznrvtElrV6yV-0gR0m7R9M-ibYbtMr5lq4V2v83_h34A_893BQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2071143691</pqid></control><display><type>article</type><title>Astrometric Observations of the Galilean Moons of Jupiter at the Pulkovo Normal Astrograph in 2016−2017</title><source>Springer Link</source><creator>Narizhnaya, N. V. ; Khovrichev, M. Yu ; Apetyan, A. A. ; Bikulova, D. A. ; Ershova, A. P. ; Balyaev, I. A. ; Kulikova, A. M. ; Os’kina, K. I. ; Maksimova, L. A.</creator><creatorcontrib>Narizhnaya, N. V. ; Khovrichev, M. Yu ; Apetyan, A. A. ; Bikulova, D. A. ; Ershova, A. P. ; Balyaev, I. A. ; Kulikova, A. M. ; Os’kina, K. I. ; Maksimova, L. A.</creatorcontrib><description>We present the results of observations of the Galilean moons of Jupiter carried out at the Normal Astrograph of the Pulkovo Observatory in 2016−2017. We obtained 761 positions of the Galilean moons of Jupiter in the system of the Gaia DR1 catalog (ICRF, J2000.0) and 854 differential coordinates of the satellites relative to each other. The mean errors in the satellites’ normal places and the corresponding root-mean-square deviations are ε
α
= 0.0020′′, ε
δ
= 0.0027′′, σ
α
= 0.0546′′, and σ
δ
= 0.0757′′. The equatorial coordinates of the moons are compared to the motion theories of planets and satellites. On average, the (O–C) residuals in the both coordinates relative to the motion theories are less than 0.031′′. The best agreement with observations is achieved by a combination of the EPM2015 and V. Lainey-V.2.0|V1.1 motion theories, which yields the average (O–C) residuals of approximately 0.02″. Peculiarities in the behavior of the (O–C) residuals and error values in Ganymede have been noticed.</description><identifier>ISSN: 0038-0946</identifier><identifier>EISSN: 1608-3423</identifier><identifier>DOI: 10.1134/S0038094618040020</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Astronomy ; Astrophysics and Astroparticles ; Astrophysics and Cosmology ; Cyclotron frequency ; Galilean satellites ; Ganymede ; Ion cyclotron radiation ; Jupiter ; Jupiter satellites ; Observations and Techniques ; Physics ; Physics and Astronomy ; Planetology ; Planets ; Satellites ; Saturn</subject><ispartof>Solar system research, 2018-07, Vol.52 (4), p.312-319</ispartof><rights>Pleiades Publishing, Inc. 2018</rights><rights>Solar System Research is a copyright of Springer, (2018). All Rights Reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-a115f33b37e06e2c2ce48006df07a5a084ee0fb6f78a1744f033900d4ca52bf33</citedby><cites>FETCH-LOGICAL-c316t-a115f33b37e06e2c2ce48006df07a5a084ee0fb6f78a1744f033900d4ca52bf33</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>315,786,790,27957,27958</link.rule.ids></links><search><creatorcontrib>Narizhnaya, N. V.</creatorcontrib><creatorcontrib>Khovrichev, M. Yu</creatorcontrib><creatorcontrib>Apetyan, A. A.</creatorcontrib><creatorcontrib>Bikulova, D. A.</creatorcontrib><creatorcontrib>Ershova, A. P.</creatorcontrib><creatorcontrib>Balyaev, I. A.</creatorcontrib><creatorcontrib>Kulikova, A. M.</creatorcontrib><creatorcontrib>Os’kina, K. I.</creatorcontrib><creatorcontrib>Maksimova, L. A.</creatorcontrib><title>Astrometric Observations of the Galilean Moons of Jupiter at the Pulkovo Normal Astrograph in 2016−2017</title><title>Solar system research</title><addtitle>Sol Syst Res</addtitle><description>We present the results of observations of the Galilean moons of Jupiter carried out at the Normal Astrograph of the Pulkovo Observatory in 2016−2017. We obtained 761 positions of the Galilean moons of Jupiter in the system of the Gaia DR1 catalog (ICRF, J2000.0) and 854 differential coordinates of the satellites relative to each other. The mean errors in the satellites’ normal places and the corresponding root-mean-square deviations are ε
α
= 0.0020′′, ε
δ
= 0.0027′′, σ
α
= 0.0546′′, and σ
δ
= 0.0757′′. The equatorial coordinates of the moons are compared to the motion theories of planets and satellites. On average, the (O–C) residuals in the both coordinates relative to the motion theories are less than 0.031′′. The best agreement with observations is achieved by a combination of the EPM2015 and V. Lainey-V.2.0|V1.1 motion theories, which yields the average (O–C) residuals of approximately 0.02″. Peculiarities in the behavior of the (O–C) residuals and error values in Ganymede have been noticed.</description><subject>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>Astrophysics and Cosmology</subject><subject>Cyclotron frequency</subject><subject>Galilean satellites</subject><subject>Ganymede</subject><subject>Ion cyclotron radiation</subject><subject>Jupiter</subject><subject>Jupiter satellites</subject><subject>Observations and Techniques</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetology</subject><subject>Planets</subject><subject>Satellites</subject><subject>Saturn</subject><issn>0038-0946</issn><issn>1608-3423</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNp1kMFOwzAQRC0EEqXwAdwscQ7s2q6THqsKCqhQJOAcOandpqRxsJ1K_AFnPpEvIWkrcUCcRtp5MysNIecIl4hcXD0D8ASGQmICAoDBAemhhCTigvFD0uvsqPOPyYn3KwAEiGWPFCMfnF3r4IqczjKv3UaFwlaeWkPDUtOJKotSq4o-2P31vqmLoB1VYQs8NeWb3Vj6aN1alXTbt3CqXtKiogxQfn9-tRKfkiOjSq_P9tonrzfXL-PbaDqb3I1H0yjnKEOkEAeG84zHGqRmOcu1SADk3ECsBgoSoTWYTJo4URgLYYDzIcBc5GrAsjbZJxe73trZ90b7kK5s46r2ZcogRhRcDrGlcEflznrvtElrV6yV-0gR0m7R9M-ibYbtMr5lq4V2v83_h34A_893BQ</recordid><startdate>20180701</startdate><enddate>20180701</enddate><creator>Narizhnaya, N. V.</creator><creator>Khovrichev, M. Yu</creator><creator>Apetyan, A. A.</creator><creator>Bikulova, D. A.</creator><creator>Ershova, A. P.</creator><creator>Balyaev, I. A.</creator><creator>Kulikova, A. M.</creator><creator>Os’kina, K. I.</creator><creator>Maksimova, L. A.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>Q9U</scope></search><sort><creationdate>20180701</creationdate><title>Astrometric Observations of the Galilean Moons of Jupiter at the Pulkovo Normal Astrograph in 2016−2017</title><author>Narizhnaya, N. V. ; Khovrichev, M. Yu ; Apetyan, A. A. ; Bikulova, D. A. ; Ershova, A. P. ; Balyaev, I. A. ; Kulikova, A. M. ; Os’kina, K. I. ; Maksimova, L. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c316t-a115f33b37e06e2c2ce48006df07a5a084ee0fb6f78a1744f033900d4ca52bf33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Astrophysics and Cosmology</topic><topic>Cyclotron frequency</topic><topic>Galilean satellites</topic><topic>Ganymede</topic><topic>Ion cyclotron radiation</topic><topic>Jupiter</topic><topic>Jupiter satellites</topic><topic>Observations and Techniques</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Planetology</topic><topic>Planets</topic><topic>Satellites</topic><topic>Saturn</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Narizhnaya, N. V.</creatorcontrib><creatorcontrib>Khovrichev, M. Yu</creatorcontrib><creatorcontrib>Apetyan, A. A.</creatorcontrib><creatorcontrib>Bikulova, D. A.</creatorcontrib><creatorcontrib>Ershova, A. P.</creatorcontrib><creatorcontrib>Balyaev, I. A.</creatorcontrib><creatorcontrib>Kulikova, A. M.</creatorcontrib><creatorcontrib>Os’kina, K. I.</creatorcontrib><creatorcontrib>Maksimova, L. A.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Database (1962 - current)</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest Science Journals</collection><collection>ProQuest Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>ProQuest Central Basic</collection><jtitle>Solar system research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Narizhnaya, N. V.</au><au>Khovrichev, M. Yu</au><au>Apetyan, A. A.</au><au>Bikulova, D. A.</au><au>Ershova, A. P.</au><au>Balyaev, I. A.</au><au>Kulikova, A. M.</au><au>Os’kina, K. I.</au><au>Maksimova, L. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Astrometric Observations of the Galilean Moons of Jupiter at the Pulkovo Normal Astrograph in 2016−2017</atitle><jtitle>Solar system research</jtitle><stitle>Sol Syst Res</stitle><date>2018-07-01</date><risdate>2018</risdate><volume>52</volume><issue>4</issue><spage>312</spage><epage>319</epage><pages>312-319</pages><issn>0038-0946</issn><eissn>1608-3423</eissn><abstract>We present the results of observations of the Galilean moons of Jupiter carried out at the Normal Astrograph of the Pulkovo Observatory in 2016−2017. We obtained 761 positions of the Galilean moons of Jupiter in the system of the Gaia DR1 catalog (ICRF, J2000.0) and 854 differential coordinates of the satellites relative to each other. The mean errors in the satellites’ normal places and the corresponding root-mean-square deviations are ε
α
= 0.0020′′, ε
δ
= 0.0027′′, σ
α
= 0.0546′′, and σ
δ
= 0.0757′′. The equatorial coordinates of the moons are compared to the motion theories of planets and satellites. On average, the (O–C) residuals in the both coordinates relative to the motion theories are less than 0.031′′. The best agreement with observations is achieved by a combination of the EPM2015 and V. Lainey-V.2.0|V1.1 motion theories, which yields the average (O–C) residuals of approximately 0.02″. Peculiarities in the behavior of the (O–C) residuals and error values in Ganymede have been noticed.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0038094618040020</doi><tpages>8</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0038-0946 |
| ispartof | Solar system research, 2018-07, Vol.52 (4), p.312-319 |
| issn | 0038-0946 1608-3423 |
| language | eng |
| recordid | cdi_proquest_journals_2071143691 |
| source | Springer Link |
| subjects | Astronomy Astrophysics and Astroparticles Astrophysics and Cosmology Cyclotron frequency Galilean satellites Ganymede Ion cyclotron radiation Jupiter Jupiter satellites Observations and Techniques Physics Physics and Astronomy Planetology Planets Satellites Saturn |
| title | Astrometric Observations of the Galilean Moons of Jupiter at the Pulkovo Normal Astrograph in 2016−2017 |
| url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-09-22T09%3A41%3A34IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Astrometric%20Observations%20of%20the%20Galilean%20Moons%20of%20Jupiter%20at%20the%20Pulkovo%20Normal%20Astrograph%20in%202016%E2%88%922017&rft.jtitle=Solar%20system%20research&rft.au=Narizhnaya,%20N.%20V.&rft.date=2018-07-01&rft.volume=52&rft.issue=4&rft.spage=312&rft.epage=319&rft.pages=312-319&rft.issn=0038-0946&rft.eissn=1608-3423&rft_id=info:doi/10.1134/S0038094618040020&rft_dat=%3Cproquest_cross%3E2071143691%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c316t-a115f33b37e06e2c2ce48006df07a5a084ee0fb6f78a1744f033900d4ca52bf33%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2071143691&rft_id=info:pmid/&rfr_iscdi=true |