Future space problems and their solutions:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Hauppauge, New York
Nova Science Publisher's, Inc.
[2017]
|
| Schlagworte: | |
| Beschreibung: | Description based on print version record and CIP data provided by publisher |
| Beschreibung: | 1 online resource |
| ISBN: | 9781536137392 1536137391 |
Internformat
MARC
| LEADER | 00000nmm a2200000zc 4500 | ||
|---|---|---|---|
| 001 | BV046098130 | ||
| 003 | DE-604 | ||
| 005 | 00000000000000.0 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 190812s2017 |||| o||u| ||||||eng d | ||
| 020 | |a 9781536137392 |9 978-1-5361-3739-2 | ||
| 020 | |a 1536137391 |9 1-5361-3739-1 | ||
| 035 | |a (ZDB-4-ENC)on1041562898 | ||
| 035 | |a (OCoLC)1041562898 | ||
| 035 | |a (DE-599)BVBBV046098130 | ||
| 040 | |a DE-604 |b ger |e rda | ||
| 041 | 0 | |a eng | |
| 082 | 0 | |a 521.01/5118 |2 23 | |
| 100 | 1 | |a Smulsky, Joseph J. |d 1944- |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Future space problems and their solutions |c Joseph J. Smulsky (Institute of Earth's Cryosphere,Tyumen Scientific Centre) |
| 264 | 1 | |a Hauppauge, New York |b Nova Science Publisher's, Inc. |c [2017] | |
| 300 | |a 1 online resource | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 500 | |a Description based on print version record and CIP data provided by publisher | ||
| 505 | 8 | |a "The emergence, existence and development of the surrounding world, both on Earth and throughout the universe, are due to the gravitational interactions of many bodies. This book is devoted to the calculation of bodies' movements in various cases of interaction that are relevant now and in the future. They are developed for the free access of the Galactica system, which is designed to provide the numerical solution for problems of the gravitational interaction of N-bodies. It tackles a whole range of problems: The optimal motion of the spacecraft, the evolution of the solar system for 100 million years, the influence of the Sun on Mercury's perihelion, the motion of near-Earth asteroids, the evolution of Earth's rotation axis, etc. As a result of solving a number of problems, new knowledge about our world was obtained. The optimal trajectory of the spacecraft approaching the Sun is determined by numerical integration of the equations of motion for spacecraft, planets, the Sun, and the Moon. Exact solutions to the problem of the Newtonian gravitational interaction of N material points moving around N2 concentric circular orbits are reviewed. Each circular orbit contains N3 located bodies and the body system rotates as an entity. Solutions in various forms were obtained. A computer program has been developed. Structures comprising up to one million bodies have been calculated. The Galactica system is used for computing movements of two asteroids: Apophis and 1950DA. The evolution of their movement over a span of 1,000 years is investigated. The moments of their closest passages near the Earth are defined. The different ways of asteroid trajectory transformations into orbits of the Earth's satellites are considered"-- | |
| 630 | 0 | 4 | |a Galactica (Computer program) |
| 650 | 7 | |a Celestial mechanics |2 fast | |
| 650 | 7 | |a Climatic changes / Mathematical models |2 fast | |
| 650 | 7 | |a Many-body problem / Numerical solutions |2 fast | |
| 650 | 7 | |a SCIENCE / Astronomy |2 bisacsh | |
| 650 | 4 | |a Many-body problem |x Numerical solutions |a Celestial mechanics |a Climatic changes |x Mathematical models | |
| 776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |a Smulsky, Joseph J., 1944- author |t Future space problems and their solutions |d Hauppauge, New York : Nova Science Publisher's, Inc., [2017] |z 9781536137385 |
| 912 | |a ZDB-4-ENC | ||
| 999 | |a oai:aleph.bib-bvb.de:BVB01-031478952 | ||
Datensatz im Suchindex
| _version_ | 1804180403133612032 |
|---|---|
| any_adam_object | |
| author | Smulsky, Joseph J. 1944- |
| author_facet | Smulsky, Joseph J. 1944- |
| author_role | aut |
| author_sort | Smulsky, Joseph J. 1944- |
| author_variant | j j s jj jjs |
| building | Verbundindex |
| bvnumber | BV046098130 |
| collection | ZDB-4-ENC |
| contents | "The emergence, existence and development of the surrounding world, both on Earth and throughout the universe, are due to the gravitational interactions of many bodies. This book is devoted to the calculation of bodies' movements in various cases of interaction that are relevant now and in the future. They are developed for the free access of the Galactica system, which is designed to provide the numerical solution for problems of the gravitational interaction of N-bodies. It tackles a whole range of problems: The optimal motion of the spacecraft, the evolution of the solar system for 100 million years, the influence of the Sun on Mercury's perihelion, the motion of near-Earth asteroids, the evolution of Earth's rotation axis, etc. As a result of solving a number of problems, new knowledge about our world was obtained. The optimal trajectory of the spacecraft approaching the Sun is determined by numerical integration of the equations of motion for spacecraft, planets, the Sun, and the Moon. Exact solutions to the problem of the Newtonian gravitational interaction of N material points moving around N2 concentric circular orbits are reviewed. Each circular orbit contains N3 located bodies and the body system rotates as an entity. Solutions in various forms were obtained. A computer program has been developed. Structures comprising up to one million bodies have been calculated. The Galactica system is used for computing movements of two asteroids: Apophis and 1950DA. The evolution of their movement over a span of 1,000 years is investigated. The moments of their closest passages near the Earth are defined. The different ways of asteroid trajectory transformations into orbits of the Earth's satellites are considered"-- |
| ctrlnum | (ZDB-4-ENC)on1041562898 (OCoLC)1041562898 (DE-599)BVBBV046098130 |
| dewey-full | 521.01/5118 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 521 - Celestial mechanics |
| dewey-raw | 521.01/5118 |
| dewey-search | 521.01/5118 |
| dewey-sort | 3521.01 45118 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03369nmm a2200397zc 4500</leader><controlfield tag="001">BV046098130</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">190812s2017 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9781536137392</subfield><subfield code="9">978-1-5361-3739-2</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">1536137391</subfield><subfield code="9">1-5361-3739-1</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ZDB-4-ENC)on1041562898</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1041562898</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV046098130</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">521.01/5118</subfield><subfield code="2">23</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Smulsky, Joseph J.</subfield><subfield code="d">1944-</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Future space problems and their solutions</subfield><subfield code="c">Joseph J. Smulsky (Institute of Earth's Cryosphere,Tyumen Scientific Centre)</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Hauppauge, New York</subfield><subfield code="b">Nova Science Publisher's, Inc.</subfield><subfield code="c">[2017]</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 online resource</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Description based on print version record and CIP data provided by publisher</subfield></datafield><datafield tag="505" ind1="8" ind2=" "><subfield code="a">"The emergence, existence and development of the surrounding world, both on Earth and throughout the universe, are due to the gravitational interactions of many bodies. This book is devoted to the calculation of bodies' movements in various cases of interaction that are relevant now and in the future. They are developed for the free access of the Galactica system, which is designed to provide the numerical solution for problems of the gravitational interaction of N-bodies. It tackles a whole range of problems: The optimal motion of the spacecraft, the evolution of the solar system for 100 million years, the influence of the Sun on Mercury's perihelion, the motion of near-Earth asteroids, the evolution of Earth's rotation axis, etc. As a result of solving a number of problems, new knowledge about our world was obtained. The optimal trajectory of the spacecraft approaching the Sun is determined by numerical integration of the equations of motion for spacecraft, planets, the Sun, and the Moon. Exact solutions to the problem of the Newtonian gravitational interaction of N material points moving around N2 concentric circular orbits are reviewed. Each circular orbit contains N3 located bodies and the body system rotates as an entity. Solutions in various forms were obtained. A computer program has been developed. Structures comprising up to one million bodies have been calculated. The Galactica system is used for computing movements of two asteroids: Apophis and 1950DA. The evolution of their movement over a span of 1,000 years is investigated. The moments of their closest passages near the Earth are defined. The different ways of asteroid trajectory transformations into orbits of the Earth's satellites are considered"--</subfield></datafield><datafield tag="630" ind1="0" ind2="4"><subfield code="a">Galactica (Computer program)</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Celestial mechanics</subfield><subfield code="2">fast</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Climatic changes / Mathematical models</subfield><subfield code="2">fast</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Many-body problem / Numerical solutions</subfield><subfield code="2">fast</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">SCIENCE / Astronomy</subfield><subfield code="2">bisacsh</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Many-body problem</subfield><subfield code="x">Numerical solutions</subfield><subfield code="a">Celestial mechanics</subfield><subfield code="a">Climatic changes</subfield><subfield code="x">Mathematical models</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe</subfield><subfield code="a">Smulsky, Joseph J., 1944- author</subfield><subfield code="t">Future space problems and their solutions</subfield><subfield code="d">Hauppauge, New York : Nova Science Publisher's, Inc., [2017]</subfield><subfield code="z">9781536137385</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-4-ENC</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-031478952</subfield></datafield></record></collection> |
| id | DE-604.BV046098130 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T08:35:12Z |
| institution | BVB |
| isbn | 9781536137392 1536137391 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-031478952 |
| oclc_num | 1041562898 |
| open_access_boolean | |
| physical | 1 online resource |
| psigel | ZDB-4-ENC |
| publishDate | 2017 |
| publishDateSearch | 2017 |
| publishDateSort | 2017 |
| publisher | Nova Science Publisher's, Inc. |
| record_format | marc |
| spelling | Smulsky, Joseph J. 1944- Verfasser aut Future space problems and their solutions Joseph J. Smulsky (Institute of Earth's Cryosphere,Tyumen Scientific Centre) Hauppauge, New York Nova Science Publisher's, Inc. [2017] 1 online resource txt rdacontent c rdamedia cr rdacarrier Description based on print version record and CIP data provided by publisher "The emergence, existence and development of the surrounding world, both on Earth and throughout the universe, are due to the gravitational interactions of many bodies. This book is devoted to the calculation of bodies' movements in various cases of interaction that are relevant now and in the future. They are developed for the free access of the Galactica system, which is designed to provide the numerical solution for problems of the gravitational interaction of N-bodies. It tackles a whole range of problems: The optimal motion of the spacecraft, the evolution of the solar system for 100 million years, the influence of the Sun on Mercury's perihelion, the motion of near-Earth asteroids, the evolution of Earth's rotation axis, etc. As a result of solving a number of problems, new knowledge about our world was obtained. The optimal trajectory of the spacecraft approaching the Sun is determined by numerical integration of the equations of motion for spacecraft, planets, the Sun, and the Moon. Exact solutions to the problem of the Newtonian gravitational interaction of N material points moving around N2 concentric circular orbits are reviewed. Each circular orbit contains N3 located bodies and the body system rotates as an entity. Solutions in various forms were obtained. A computer program has been developed. Structures comprising up to one million bodies have been calculated. The Galactica system is used for computing movements of two asteroids: Apophis and 1950DA. The evolution of their movement over a span of 1,000 years is investigated. The moments of their closest passages near the Earth are defined. The different ways of asteroid trajectory transformations into orbits of the Earth's satellites are considered"-- Galactica (Computer program) Celestial mechanics fast Climatic changes / Mathematical models fast Many-body problem / Numerical solutions fast SCIENCE / Astronomy bisacsh Many-body problem Numerical solutions Celestial mechanics Climatic changes Mathematical models Erscheint auch als Druck-Ausgabe Smulsky, Joseph J., 1944- author Future space problems and their solutions Hauppauge, New York : Nova Science Publisher's, Inc., [2017] 9781536137385 |
| spellingShingle | Smulsky, Joseph J. 1944- Future space problems and their solutions "The emergence, existence and development of the surrounding world, both on Earth and throughout the universe, are due to the gravitational interactions of many bodies. This book is devoted to the calculation of bodies' movements in various cases of interaction that are relevant now and in the future. They are developed for the free access of the Galactica system, which is designed to provide the numerical solution for problems of the gravitational interaction of N-bodies. It tackles a whole range of problems: The optimal motion of the spacecraft, the evolution of the solar system for 100 million years, the influence of the Sun on Mercury's perihelion, the motion of near-Earth asteroids, the evolution of Earth's rotation axis, etc. As a result of solving a number of problems, new knowledge about our world was obtained. The optimal trajectory of the spacecraft approaching the Sun is determined by numerical integration of the equations of motion for spacecraft, planets, the Sun, and the Moon. Exact solutions to the problem of the Newtonian gravitational interaction of N material points moving around N2 concentric circular orbits are reviewed. Each circular orbit contains N3 located bodies and the body system rotates as an entity. Solutions in various forms were obtained. A computer program has been developed. Structures comprising up to one million bodies have been calculated. The Galactica system is used for computing movements of two asteroids: Apophis and 1950DA. The evolution of their movement over a span of 1,000 years is investigated. The moments of their closest passages near the Earth are defined. The different ways of asteroid trajectory transformations into orbits of the Earth's satellites are considered"-- Galactica (Computer program) Celestial mechanics fast Climatic changes / Mathematical models fast Many-body problem / Numerical solutions fast SCIENCE / Astronomy bisacsh Many-body problem Numerical solutions Celestial mechanics Climatic changes Mathematical models |
| title | Future space problems and their solutions |
| title_auth | Future space problems and their solutions |
| title_exact_search | Future space problems and their solutions |
| title_full | Future space problems and their solutions Joseph J. Smulsky (Institute of Earth's Cryosphere,Tyumen Scientific Centre) |
| title_fullStr | Future space problems and their solutions Joseph J. Smulsky (Institute of Earth's Cryosphere,Tyumen Scientific Centre) |
| title_full_unstemmed | Future space problems and their solutions Joseph J. Smulsky (Institute of Earth's Cryosphere,Tyumen Scientific Centre) |
| title_short | Future space problems and their solutions |
| title_sort | future space problems and their solutions |
| topic | Galactica (Computer program) Celestial mechanics fast Climatic changes / Mathematical models fast Many-body problem / Numerical solutions fast SCIENCE / Astronomy bisacsh Many-body problem Numerical solutions Celestial mechanics Climatic changes Mathematical models |
| topic_facet | Galactica (Computer program) Celestial mechanics Climatic changes / Mathematical models Many-body problem / Numerical solutions SCIENCE / Astronomy Many-body problem Numerical solutions Celestial mechanics Climatic changes Mathematical models |
| work_keys_str_mv | AT smulskyjosephj futurespaceproblemsandtheirsolutions |