Voyager 1: Perbedaan antara revisi
Konten dihapus Konten ditambahkan
Baris 13:
Secara resmi NASA telah menyatakan bahwa Voyager 1 telah meninggalkan tata surya dan kini berada di Interstellar space atau ruang antar bintang.
==== Instrumen ilmiah ====
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! scope="col" style="width:135px;"| Instrument Name
! scope="col" style="width:50px;"| Abr.
<!-- ! scope="col" width="50" | Image -->
! Description
|-
| style="text-align:center" |Imaging Science System <br>{{color|#E62020|{{small|('''disabled''')}}}}
| style="text-align:center" |('''ISS''')
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| Dimanfaatkan sistem dua kamera (narrow-angle/wide-angle) untuk memberikan citra Jupiter, Saturnus dan benda-benda lainnya di sepanjang lintasan. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-01 '''More''']
{| class="wikitable collapsible"
|-
! colspan="2" | Filters
|-
|
{| style="text-align:center"
! colspan="4" scope="col" style="width:320px;"| Narrow Angle Camera Filters<ref name="NACam">{{cite web |url=http://pds-rings.seti.org/voyager/iss/inst_cat_na1.html#filters |title=Voyager 1 Narrow Angle Camera Description |publisher=NASA |accessdate=January 17, 2011 }}</ref>
|-
! scope="col" style="background:#e5e5e5; width:60px;"| Name
! style="background: #e5e5e5" | Wavelength
! style="background: #e5e5e5" | Spectrum
! style="background: #e5e5e5" | Sensitivity
|-
| Clear
| 280–640 nm
| [[File:Voyager - Filters - Clear.png|50px | center]]
| style="background:#fff;"|
|-
| [[Ultraviolet|UV]]
| 280–370 nm
| [[File:Voyager - Filters - UV.png|50px | center]]
| style="background: #1d0036" |
|-
| Violet
| 350–450 nm
| [[File:Voyager - Filters - Violet.png|50px | center]]
| style="background: #8300b5" |
|-
| Blue
| 430–530 nm
| [[File:Voyager - Filters - Blue.png|50px | center]]
| style="background: #00d5ff" |
|-
| '
| '
| [[File:Clear.png|50px | center]]
| '
|-
| Green
| 530–640 nm
| [[File:Voyager - Filters - Green.png|50px | center]]
| style="background: #ffef00" |
|-
| '
| '
| style="text-align:center" |[[File:Clear.png|50px | center]]
| '
|-
| Orange
| 590–640 nm
| [[File:Voyager - Filters - Orange.png|50px | center]]
| style="background: #ff8900" |
|-
| '
| '
| [[File:Clear.png|50px | center]]
| '
|}
|
{| style="text-align:center"
! colspan="4" scope="col" style="width:320px;"| Wide Angle Camera Filters<ref name="WACam">{{cite web |url=http://pds-rings.seti.org/voyager/iss/inst_cat_wa1.html#filters |title=Voyager 1 Wide Angle Camera Description |publisher=NASA |accessdate=January 17, 2011 }}</ref>
|-
! scope="col" style="background:#e5e5e5; width:60px;"| Name
! style="background: #e5e5e5" | Wavelength
! style="background: #e5e5e5" | Spectrum
! style="background: #e5e5e5" | Sensitivity
|-
| Clear
| 280–640 nm
| [[File:Voyager - Filters - Clear.png|50px | center]]
| style="background:#fff;"|
|-
| '
| '
| [[File:Clear.png|50px | center]]
| '
|-
| Violet
| 350–450 nm
| [[File:Voyager - Filters - Violet.png|50px | center]]
| style="background: #8300b5" |
|-
| Blue
| 430–530 nm
| [[File:Voyager - Filters - Blue.png|50px | center]]
| style="background: #00d5ff" |
|-
| [[Methane|CH<sub>4</sub>]]-U
| 536–546 nm
| [[File:Voyager - Filters - CH4U.png|50px | center]]
| style="background: #81ff00" |
|-
| Green
| 530–640 nm
| [[File:Voyager - Filters - Green.png|50px | center]]
| style="background: #ffef00" |
|-
| [[Sodium|Na]]-D
| 588–590 nm
| [[File:Voyager - Filters - NaD.png|50px | center]]
| style="background: #ffe200" |
|-
| Orange
| 590–640 nm
| [[File:Voyager - Filters - Orange.png|50px | center]]
| style="background: #ff8900" |
|-
| [[Methane|CH<sub>4</sub>]]-JST
| 614–624 nm
| [[File:Voyager - Filters - CH4JST.png|50px | center]]
| 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|('''disabled''')}}}}
| style="text-align:center" |('''RSS''')
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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|('''disabled''')}}}}
| style="text-align:center" |('''IRIS''')
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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]}}
|-
| style="text-align:center" |Ultraviolet [[Spectrometer]] <br>{{color|#4CBB17|{{small|('''active''')}}}}
| style="text-align:center" |('''UVS''')
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| Dirancang untuk mengukur sifat atmosfer, dan untuk mengukur radiasi. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-04 '''More''']
* {{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|('''active''')}}}}
| style="text-align:center" |('''MAG''')
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| Dirancang untuk menyelidiki medan magnet Jupiter dan Saturnus, interaksi angin surya dengan magnetospheres planet ini, dan medan magnet dari ruang antarplanet ke batas antara angin matahari dan medan magnet ruang antarbintang, jika menyeberang. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-05 '''More''']
* {{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" |[[Plasma (physics)|Plasma]] [[Spectrometer]] <br>{{color|#f93|{{small|('''defective''')}}}}
| 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|('''active''')}}}}
| style="text-align:center" |('''LECP''')
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| Mengukur diferensial dalam fluks energi dan distribusi sudut ion, elektron dan diferensial dalam komposisi ion energi. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-07 '''More''']
* {{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" |[[Cosmic Ray]] System <br>{{color|#4CBB17|{{small|('''active''')}}}}
| style="text-align:center" |('''CRS''')
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| Menentukan asal dan proses percepatan, riwayat hidup, dan kontribusi dinamis sinar kosmik antar bintang, nukleosintesis elemen dalam sumber kosmik-ray, perilaku sinar kosmik dalam medium antarplanet, dan planet terjebak energik-lingkungan partikel. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-08 '''More''']
* {{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" |Planetary [[Radio Astronomy]] Investigation <br>{{color|#E62020|{{small|('''disabled''')}}}}
| 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" |[[Polarimeter|Photopolarimeter]] System <br>{{color|#f93|{{small|('''defective''')}}}}
| 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" |[[Plasma (physics)|Plasma]] Wave System <br>{{color|#4CBB17|{{small|('''active''')}}}}
| style="text-align:center" |('''PWS''')
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| Menyediakan kontinu, pengukuran selubung-independen dari profil elektron-density di Jupiter dan Saturnus serta informasi dasar tentang interaksi gelombang-partikel lokal, berguna dalam mempelajari magnetospheres. [http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1977-084A-13 '''More''']
* {{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]}}
|}
== Referensi ==
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