Voyager 1: Perbedaan antara revisi

{{Infobox spaceflight

| name = Voyager 1

| image = Voyager spacecraft model.png

| image_alt = Model pesawat ruang angkasa Voyager, pesawat ruang angkasa bertubuh kecil dengan antena besar dan banyak lengan serta antena yang memanjang darinya

| website = {{url|https://voyager.jpl.nasa.gov/}}

| COSPAR_ID = 1977-084A<ref name="nasa.084A">{{cite web |url=https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1977-084A |title=Voyager 1 |publisher=NASA/NSSDC |work=NSSDC Master Catalog |accessdate=26 Desember 2019 |df=mdy-all}}</ref>

| SATCAT = 10321<ref name="n2yo.10321">{{cite web |url=https://www.n2yo.com/satellite/?s=10321 |title=Voyager 1 |publisher=N2YO |accessdate=26 Desember 2019}}</ref>

| mission_duration = {{plainlist|

}}

| manufacturer = Jet Propulsion Laboratory

| power = 470&nbsp;watt (saat peluncuran)

| launch_rocket = [[Titan IIIE]]

| last_contact = <!-- {{end-date|[date]}} -->

| type = flyby

| object = [[Jupiter]]

| arrival_date = 12 November 1980

}}

| programme = [[Program Flagship|Flagship]]

| previous_mission = ''[[Voyager 2]]''

}}

 

 

Sasaran wahana ini termasuk penerbangan melintasi [[Jupiter]], [[Saturnus]], dan satelit terbesar Saturnus, [[Titan (satelit)|Titan]]. Meskipun perjalanan wahana ini dapat diubah agar dapat melewati [[Pluto]] dengan membatalkan penerbangan melintasi Titan, penjelajahan satelit tersebut menjadi prioritas karena memiliki atmosfer substansial.<ref name="faq"/><ref>{{cite web |url=https://www.nasaspaceflight.com/2015/07/new-horizons-pluto-historic-kuiper-encounter/ |title=New Horizons conducts flyby of Pluto in historic Kuiper Belt encounter |accessdate=2 September 2015}}</ref><ref name="SD">{{cite web |url=http://www.spacedaily.com/reports/What_If_Voyager_Had_Explored_Pluto_999.html |title=What If Voyager Had Explored Pluto? |accessdate=2 September 2015}}</ref> Voyager 1 mempelajari cuaca, medan magnet, dan cincin dari dua planet sekaligus merupakan wahana pertama yang menunjukkan citra-citra terperinci [[satelit alami]] kedua planet tersebut.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

{| class="wikitable"

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! scope="col" style="width:135px;"| Nama Instrumen

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! Deskripsi

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{| class="wikitable collapsible"

| Clear

| 280–640&nbsp;nm

| style="background:#fff;"|

|-

| [[Ultraviolet|UV]]

| 280–370&nbsp;nm

| style="background: #1d0036" |

|-

| Violet

| 350–450&nbsp;nm

| style="background: #8300b5" |

|-

| Blue

| 430–530&nbsp;nm

| style="background: #00d5ff" |

|-

| '

| '

| '

|-

| Green

| 530–640&nbsp;nm

| style="background: #ffef00" |

|-

| '

| '

| '

|-

| Orange

| 590–640&nbsp;nm

| style="background: #ff8900" |

|-

| '

| '

| '

|}

| Clear

| 280–640&nbsp;nm

| style="background:#fff;"|

|-

| '

| '

| '

|-

| Violet

| 350–450&nbsp;nm

| style="background: #8300b5" |

|-

| Blue

| 430–530&nbsp;nm

| style="background: #00d5ff" |

|-

| [[Methane|CH₄]]-U

| 536–546&nbsp;nm

| style="background: #81ff00" |

|-

| Green

| 530–640&nbsp;nm

| style="background: #ffef00" |

|-

| [[Sodium|Na]]-D

| 588–590&nbsp;nm

| style="background: #ffe200" |

|-

| Orange

| 590–640&nbsp;nm

| style="background: #ff8900" |

|-

| [[Methane|CH₄]]-JST

| 614–624&nbsp;nm

| style="background: #ff7b00" |

|}

|}

 

* {{small|'''Principal investigator:''' Bradford Smith / University of Arizona }} ([http://pds-rings.seti.org/voyager/iss/index.html PDS/PRN website])

* {{small|'''Data:''' [http://pds-imaging.jpl.nasa.gov/Admin/resources/cd_voyager.html PDS/PDI data catalog], [http://pds-rings.seti.org/voyager/iss/raw_images.html PDS/PRN data catalog]}}

|-

| style="text-align:center" |Radio Science System <br>{{color|#E62020|{{small|('''dimatikan''')}}}}

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| Memanfaatkan sistem telekomunikasi dari pesawat ruang angkasa Voyager untuk menentukan sifat fisik planet dan satelit (ionosfer, atmosfer, massa, bidang gravitasi, kepadatan) dan jumlah dan distribusi ukuran materi dalam cincin Saturnus dan dimensi cincin. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-02 '''More''']

* {{small|'''Peneliti utama:''' G. Tyler / Stanford University [http://pds-rings.seti.org/voyager/iss/instrument.html PDS/PRN overview]}}

* {{small|1='''Data:''' [http://ppi.pds.nasa.gov/search/?filter=VG_230,VG_231,VG_232,VG_233&title=Voyager_1_Radio_Science_Investigation PDS/PPI data catalog], [http://pds-rings.seti.org/voyager/rss/index.html PDS/PRN data catalog] '''('''[http://pds-rings.seti.org/vol/VG_28xx_peer_review/VG_2803/ VG_2803]''')''', [http://nssdcftp.gsfc.nasa.gov/spacecraft_data/voyager/voyager1/radio_science_rss/ NSSDC data archive]}}

|-

| style="text-align:center" |Infrared [[Interferometer]] [[Spectrometer]] <br>{{color|#E62020|{{small|('''dimatikan''')}}}}

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| Menelaah keseimbangan energi global dan lokal dan komposisi atmosfer. Profil suhu vertikal juga diperoleh dari planet-planet dan satelit serta komposisi, sifat termal, dan ukuran partikel dalam cincin Saturnus. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-03 '''More''']

* {{small|'''Peneliti utama:''' Rudolf Hanel / NASA Goddard Space Flight Center ([http://pds-rings.seti.org/voyager/iris/instrument.html PDS/PRN website])}}

* {{small|'''Data:''' [http://pds-rings.seti.org/voyager/iris/original_volume.html PDS/PRN data catalog], [http://pds-rings.seti.org/voyager/iris/expanded_volumes.html PDS/PRN expanded data catalog] '''('''[http://pds-rings.seti.org/vol/VGIRIS_xxxx_peer_review/VGIRIS_0001/ VGIRIS_0001], [http://pds-rings.seti.org/vol/VGIRIS_xxxx_peer_review/VGIRIS_0002/ VGIRIS_002]''')''', [http://nssdcftp.gsfc.nasa.gov/spacecraft_data/voyager/voyager1/infrared_interferometer_spectrometer_iris/ NSSDC Jupiter data archive]}}

* {{small|'''Peneliti utama:''' A. Broadfoot / University of Southern California ([http://pds-rings.seti.org/voyager/uvs/instrument.html PDS/PRN website])}}

* {{small|'''Data:''' [http://pds-rings.seti.org/voyager/uvs/data.html PDS/PRN data catalog]}}

|-

| style="text-align:center" |Triaxial Fluxgate [[Magnetometer]] <br>{{color|#4CBB17|{{small|('''aktif''')}}}}

* {{small|'''Peneliti utama:''' Norman Ness / NASA Goddard Space Flight Center ([http://vgrmag.gsfc.nasa.gov/ website])}}

* {{small|1='''Data:''' [http://ppi.pds.nasa.gov/search/?filter=VG_1501,VG_1601,VGMA_1&title=Voyager_1_Magnetometer_Investigation PDS/PPI data catalog], [http://nssdcftp.gsfc.nasa.gov/spacecraft_data/voyager/voyager1/magnetic_fields/ NSSDC data archive]}}

|-

| style="text-align:center" |('''PLS''')

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| Menyelidiki sifat makroskopik dari ion plasma dan langkah-langkah elektron dalam kisaran energi dari 5 eV sampai 1 keV. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-06 '''More''']

* {{small|'''Peneliti utama:''' John Richardson / MIT ([http://web.mit.edu/space/www/voyager/voyager.html website])}}

* {{small|1='''Data:''' [http://ppi.pds.nasa.gov/search/?filter=VG_1501,VG_1601,VG_PLS&title=Voyager_1_Plasma_Science_Investigation PDS/PPI data catalog], [http://nssdcftp.gsfc.nasa.gov/spacecraft_data/voyager/voyager1/plasma/ NSSDC data archive]}}

|-

| style="text-align:center" |Low Energy [[Charged Particle]] Instrument <br>{{color|#4CBB17|{{small|('''aktif''')}}}}

* {{small|'''Peneliti utama:''' Stamatios Krimigis / JHU/APL / University of Maryland ([http://sd-www.jhuapl.edu/VOYAGER/ JHU/APL website] / [http://space.umd.edu/Voyager/ UMD website] / [http://voyager.ftecs.com/default.htm KU website])}}

* {{small|1='''Data:''' [http://voyager-mac.umd.edu/ UMD data plotting], [http://ppi.pds.nasa.gov/search/?filter=VG_1501,VG_1601,VGLE_&title=Voyager_1_Low-Energy_Charge_Particle_Investigation_at_Saturn PDS/PPI data catalog], [http://nssdcftp.gsfc.nasa.gov/spacecraft_data/voyager/voyager1/particle/lecp/ NSSDC data archive]}}

|-

| style="text-align:center" |('''CRS''')

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* {{small|'''Peneliti utama:''' [[Edward C. Stone|Edward Stone]] / Caltech / NASA Goddard Space Flight Center ([http://voyager.gsfc.nasa.gov/ website])}}

* {{small|1='''Data:''' [http://ppi.pds.nasa.gov/search/?filter=VG_1501,VG_1601&title=Voyager_1_Cosmic_Ray_Investigation PDS/PPI data catalog], [http://nssdcftp.gsfc.nasa.gov/spacecraft_data/voyager/voyager1/particle/crs/ NSSDC data archive]}}

|-

| style="text-align:center" |('''PRA''')

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| Memanfaatkan frekuensi radio penerima menyapu untuk mempelajari sinyal radio-emisi dari Jupiter dan Saturnus. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-10 '''More''']

* {{small|'''Peneliti utama:''' James Warwick / University of Colorado}}

* {{small|1='''Data:''' [http://ppi.pds.nasa.gov/search/?filter=VG_1501,VG_1601,VGPR_1201&title=Voyager_1_Planetary_Radio_Astronomy_Investigation PDS/PPI data catalog], [http://nssdcftp.gsfc.nasa.gov/spacecraft_data/voyager/voyager1/planet_radio_ast_pra/planetary_radio_%20astronomy_data/ NSSDC data archive]}}

|-

| style="text-align:center" |('''PPS''')

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| Memanfaatkan teleskop dengan polarizer untuk mengumpulkan informasi tentang tekstur permukaan dan komposisi Jupiter dan Saturnus dan informasi tentang sifat hamburan atmosfer dan kepadatan untuk kedua planet. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-11 '''More''']

* {{small|'''Peneliti utama:''' Arthur Lane / JPL ([http://pds-rings.seti.org/voyager/pps/instrument.html PDS/PRN website])}}

* {{small|'''Data:''' [http://pds-rings.seti.org/voyager/pps/data.html PDS/PRN data catalog]}}

|-

| style="text-align:center" |('''PWS''')

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* {{small|'''Peneliti utama:''' Donald Gurnett / University of Iowa ([http://www-pw.physics.uiowa.edu/plasma-wave/voyager/ website])}}

* {{small|'''Data:''' [http://ppi.pds.nasa.gov/search/voyager1/voyager1_pws.jsp PDS/PPI data catalog]}}

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== Referensi ==

== Pranala luar ==

* {{en}} [http://voyager.jpl.nasa.gov Situs ''Voyager'' dari NASA]

{{Program Voyager}}

 

[[Kategori:Wahana antariksa yang diluncurkan tahun 1977]]

[[Kategori:Wahana antariksa NASA]]