Benjamin P Weiss, José M G Merayo, Jodie B Ream, Rona Oran, Peter Brauer, Corey J Cochrane, Kyle Cloutier, Linda T Elkins-Tanton, John L Jørgensen, Clara Maurel, Ryan S Park, Carol A Polanskey, Maria de Soria Santacruz-Pich, Carol A Raymond, Christopher T Russell, Daniel Wenkert, Mark A Wieczorek, Maria T Zuber
{"title":"心理磁力调查","authors":"Benjamin P Weiss, José M G Merayo, Jodie B Ream, Rona Oran, Peter Brauer, Corey J Cochrane, Kyle Cloutier, Linda T Elkins-Tanton, John L Jørgensen, Clara Maurel, Ryan S Park, Carol A Polanskey, Maria de Soria Santacruz-Pich, Carol A Raymond, Christopher T Russell, Daniel Wenkert, Mark A Wieczorek, Maria T Zuber","doi":"10.1007/s11214-023-00965-z","DOIUrl":null,"url":null,"abstract":"<p><p>The objective of the Psyche Magnetometry Investigation is to test the hypothesis that asteroid (16) Psyche formed from the core of a differentiated planetesimal. To address this, the Psyche Magnetometer will measure the magnetic field around the asteroid to search for evidence of remanent magnetization. Paleomagnetic measurements of meteorites and dynamo theory indicate that a diversity of planetesimals once generated dynamo magnetic fields in their metallic cores. Likewise, the detection of a strong magnetic moment ( <math><mo>></mo> <mn>2</mn> <mo>×</mo> <msup><mrow><mn>10</mn></mrow> <mrow><mn>14</mn></mrow> </msup> <mspace></mspace> <msup><mtext>Am</mtext> <mn>2</mn></msup> </math> ) at Psyche would likely indicate that the body once generated a core dynamo, implying that it formed by igneous differentiation. The Psyche Magnetometer consists of two three-axis fluxgate Sensor Units (SUs) mounted 0.7 m apart along a 2.15-m long boom and connected to two Electronics Units (EUs) located within the spacecraft bus. The Magnetometer samples at up to 50 Hz, has a range of <math><mo>±</mo> <mn>80</mn> <mo>,</mo> <mn>000</mn> <mspace></mspace> <mtext>nT</mtext></math> , and an instrument noise of <math><mn>39</mn> <mspace></mspace> <mtext>pT</mtext> <mspace></mspace> <msup><mtext>axis</mtext> <mrow><mo>-</mo> <mn>1</mn></mrow> </msup> <mspace></mspace> <mn>3</mn> <mi>σ</mi></math> integrated over 0.1 to 1 Hz. The two pairs of SUs and EUs provide redundancy and enable gradiometry measurements to suppress noise from flight system magnetic fields. The Magnetometer will be powered on soon after launch and acquire data for the full duration of the mission. The ground data system processes the Magnetometer measurements to obtain an estimate of Psyche's dipole moment.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"219 3","pages":"22"},"PeriodicalIF":9.1000,"publicationDate":"2023-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10049963/pdf/","citationCount":"0","resultStr":"{\"title\":\"The Psyche Magnetometry Investigation.\",\"authors\":\"Benjamin P Weiss, José M G Merayo, Jodie B Ream, Rona Oran, Peter Brauer, Corey J Cochrane, Kyle Cloutier, Linda T Elkins-Tanton, John L Jørgensen, Clara Maurel, Ryan S Park, Carol A Polanskey, Maria de Soria Santacruz-Pich, Carol A Raymond, Christopher T Russell, Daniel Wenkert, Mark A Wieczorek, Maria T Zuber\",\"doi\":\"10.1007/s11214-023-00965-z\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p><p>The objective of the Psyche Magnetometry Investigation is to test the hypothesis that asteroid (16) Psyche formed from the core of a differentiated planetesimal. To address this, the Psyche Magnetometer will measure the magnetic field around the asteroid to search for evidence of remanent magnetization. Paleomagnetic measurements of meteorites and dynamo theory indicate that a diversity of planetesimals once generated dynamo magnetic fields in their metallic cores. Likewise, the detection of a strong magnetic moment ( <math><mo>></mo> <mn>2</mn> <mo>×</mo> <msup><mrow><mn>10</mn></mrow> <mrow><mn>14</mn></mrow> </msup> <mspace></mspace> <msup><mtext>Am</mtext> <mn>2</mn></msup> </math> ) at Psyche would likely indicate that the body once generated a core dynamo, implying that it formed by igneous differentiation. The Psyche Magnetometer consists of two three-axis fluxgate Sensor Units (SUs) mounted 0.7 m apart along a 2.15-m long boom and connected to two Electronics Units (EUs) located within the spacecraft bus. The Magnetometer samples at up to 50 Hz, has a range of <math><mo>±</mo> <mn>80</mn> <mo>,</mo> <mn>000</mn> <mspace></mspace> <mtext>nT</mtext></math> , and an instrument noise of <math><mn>39</mn> <mspace></mspace> <mtext>pT</mtext> <mspace></mspace> <msup><mtext>axis</mtext> <mrow><mo>-</mo> <mn>1</mn></mrow> </msup> <mspace></mspace> <mn>3</mn> <mi>σ</mi></math> integrated over 0.1 to 1 Hz. The two pairs of SUs and EUs provide redundancy and enable gradiometry measurements to suppress noise from flight system magnetic fields. The Magnetometer will be powered on soon after launch and acquire data for the full duration of the mission. The ground data system processes the Magnetometer measurements to obtain an estimate of Psyche's dipole moment.</p>\",\"PeriodicalId\":21902,\"journal\":{\"name\":\"Space Science Reviews\",\"volume\":\"219 3\",\"pages\":\"22\"},\"PeriodicalIF\":9.1000,\"publicationDate\":\"2023-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10049963/pdf/\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Space Science Reviews\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1007/s11214-023-00965-z\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"2023/3/28 0:00:00\",\"PubModel\":\"Epub\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Space Science Reviews","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1007/s11214-023-00965-z","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2023/3/28 0:00:00","PubModel":"Epub","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
The objective of the Psyche Magnetometry Investigation is to test the hypothesis that asteroid (16) Psyche formed from the core of a differentiated planetesimal. To address this, the Psyche Magnetometer will measure the magnetic field around the asteroid to search for evidence of remanent magnetization. Paleomagnetic measurements of meteorites and dynamo theory indicate that a diversity of planetesimals once generated dynamo magnetic fields in their metallic cores. Likewise, the detection of a strong magnetic moment ( ) at Psyche would likely indicate that the body once generated a core dynamo, implying that it formed by igneous differentiation. The Psyche Magnetometer consists of two three-axis fluxgate Sensor Units (SUs) mounted 0.7 m apart along a 2.15-m long boom and connected to two Electronics Units (EUs) located within the spacecraft bus. The Magnetometer samples at up to 50 Hz, has a range of , and an instrument noise of integrated over 0.1 to 1 Hz. The two pairs of SUs and EUs provide redundancy and enable gradiometry measurements to suppress noise from flight system magnetic fields. The Magnetometer will be powered on soon after launch and acquire data for the full duration of the mission. The ground data system processes the Magnetometer measurements to obtain an estimate of Psyche's dipole moment.
期刊介绍:
Space Science Reviews (SSRv) stands as an international journal dedicated to scientific space research, offering a contemporary synthesis across various branches of space exploration. Emphasizing scientific outcomes and instruments, SSRv spans astrophysics, physics of planetary systems, solar physics, and the physics of magnetospheres & interplanetary matter.
Beyond Topical Collections and invited Review Articles, Space Science Reviews welcomes unsolicited Review Articles and Special Communications. The latter encompass papers related to a prior topical volume/collection, report-type papers, or timely contributions addressing a robust combination of space science and technology. These papers succinctly summarize both the science and technology aspects of instruments or missions in a single publication.