<?xml version="1.0" encoding="UTF-8"?>
<CourseUnit xmlns="http://www.manchester.ac.uk/CUICourseUnitDetails" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.manchester.ac.uk/CUICourseUnitDetails.xsd">
  <UnitCode Applicant="Y" Label="Unit code" Student="Y">
    <Code>PHYS10191</Code>
  </UnitCode>
  <UnitTitle Applicant="Y" Label="Unit title" Student="Y">
    <Title>Introduction to Astrophysics and Cosmology</Title>
  </UnitTitle>
  <MaxUnits Applicant="Y" Label="Credit rating" Student="Y">
    <Units>10</Units>
  </MaxUnits>
  <TeachingPeriods Applicant="Y" Label="Teaching period(s)" Student="Y">
    <Period>Semester 1</Period>
  </TeachingPeriods>
  <AcademicCareer Applicant="Y" Label="Academic career" Student="Y">
    <Value>Undergraduate</Value>
  </AcademicCareer>
  <UnitLevel Applicant="Y" Label="Unit level" Student="Y">
    <Level>Level 1</Level>
  </UnitLevel>
  <StaffList Applicant="Y" Label="Teaching staff" RoleLabel="Course Unit Role" Student="Y">
    <StaffMember>
      <Name>Laura Wolz</Name>
      <Role>Unit coordinator</Role>
    </StaffMember>
  </StaffList>
  <OfferedBy Applicant="Y" Label="Offered by" Student="Y">
    <OrganisationList>
      <Organisation>
        <OrgName>Department of Physics &amp; Astronomy</OrgName>
      </Organisation>
    </OrganisationList>
    <GroupList>
      <Group>
        <GroupName></GroupName>
      </Group>
    </GroupList>
    <FheqLevels>
      <FheqLevel>
        <LevelNumber>1</LevelNumber>
        <LevelName>FHEQ level (Framework for Higher Education Qualifications) ' First part HE study/Bachelors ' </LevelName>
      </FheqLevel>
    </FheqLevels>
    <Ects>
      <MaxUnits>European Credit Transfer &amp; Accumulation System Rating :   5.0</MaxUnits>
    </Ects>
  </OfferedBy>
  <MarketingOverview Applicant="Y" Label="Marketing Course unit overview" Student="">
    <Content>&lt;p&gt;This unit introduces basic concepts of astronomy and cosmology. The unit introduces the physical scale of the Universe and astronomical objects including appropriate use of astronomical units. The laws of gravity will be introduced in the context of astronomical objects and their movements, including a brief overview of Kepler’s laws. Observational aspects are discussed which includes properties of light and Blackbody radiation, a revision of geometric optics, introduction of telescope design, spectroscopy and basic concepts of detectors. The unit introduces observational concepts of distance measurements for geometric as well as brightness distances. The properties and basic life cycle of stars are discussed using the Hertzsprung Russell diagram, stellar structure, hydrostatic equilibrium, energy production including nucleosynthesis, and stellar remnants. The basic properties and structure of galaxies are introduced with galaxy type classification. Galactic rotational curves and evidence for dark matter are demonstrated. The unit concludes with a chapter on cosmology which introduces the concept of redshift, observational evidence or the Big Bang including the Hubble flow, a basic derivation of the first Friedmann equation and an evaluation of the Friedmann equation for cosmological components, as well as physics of the early universe. &amp;nbsp;&lt;/p&gt;</Content>
  </MarketingOverview>
  <UnitOverview Applicant="" Label="Course unit overview" Student="Y">
    <Content>&lt;p&gt;This unit introduces basic concepts of astronomy and cosmology. The unit introduces the physical scale of the Universe and astronomical objects including appropriate use of astronomical units. The laws of gravity will be introduced in the context of astronomical objects and their movements, including a brief overview of Kepler’s laws. Observational aspects are discussed which includes properties of light and Blackbody radiation, a revision of geometric optics, introduction of telescope design, spectroscopy and basic concepts of detectors. The unit introduces observational concepts of distance measurements for geometric as well as brightness distances. The properties and basic life cycle of stars are discussed using the Hertzsprung Russell diagram, stellar structure, hydrostatic equilibrium, energy production including nucleosynthesis, and stellar remnants. The basic properties and structure of galaxies are introduced with galaxy type classification. Galactic rotational curves and evidence for dark matter are demonstrated. The unit concludes with a chapter on cosmology which introduces the concept of redshift, observational evidence or the Big Bang including the Hubble flow, a basic derivation of the first Friedmann equation and an evaluation of the Friedmann equation for cosmological components, as well as physics of the early universe. &amp;nbsp;&lt;/p&gt;</Content>
  </UnitOverview>
  <Aims Applicant="Y" Label="Aims" Student="Y">
    <Content>&lt;p&gt;This course aims to introduce the physical properties of stars and galaxies, observational concepts of astronomy, application of basic physical laws including gravitation to explain the properties of astronomical objects and basic concepts of cosmology and observational evidence.&lt;/p&gt;</Content>
  </Aims>
  <LearningOutcomes Applicant="Y" Label="Learning outcomes" Student="Y">
    <Content>&lt;p class="MsoNormal" style="line-height:normal;"&gt;On completion successful students will be able to:&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Use the equations which describe the evolution of the Universe to derive properties of the Universe&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Describe the fundamental constituents of the Universe: baryons, dark matter and dark energy, and the observational evidence for their presence&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Describe and explain the evolution of our Universe, including the evidence for the Big Bang&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Explain how astronomical distances are measured&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Describe the structure of the Milky Way and other galaxies&amp;nbsp;&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Apply the laws of gravity to astrophysical objects&amp;nbsp;&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Describe and explain the physics of detectors and telescopes including geometric optics&amp;nbsp;&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Use the basic laws of physics to explain the global properties and basic evolution of stars&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Use the basic laws of physics to explain the global properties and basic evolution of stars&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Carry out calculations in using common astrophysical units&lt;/p&gt;&lt;p style="margin-left:36pt;"&gt;&amp;nbsp;&lt;/p&gt;</Content>
  </LearningOutcomes>
  <Knowledge Applicant="Y" Label="Knowledge and understanding" Student="Y">
    <Content></Content>
  </Knowledge>
  <IntellectualSkills Applicant="Y" Label="Intellectual skills" Student="Y">
    <Content></Content>
  </IntellectualSkills>
  <PracticalSkills Applicant="Y" Label="Practical skills" Student="Y">
    <Content></Content>
  </PracticalSkills>
  <TransferableSkills Applicant="Y" Label="Transferable skills and personal qualities" Student="Y">
    <Content></Content>
  </TransferableSkills>
  <EmployabilitySkillsList Applicant="Y" Label="Employability skills" Student="Y">
    <Skill>
      <SkillId></SkillId>
      <SkillDescription></SkillDescription>
    </Skill>
  </EmployabilitySkillsList>
  <Syllabus Applicant="Y" Label="Syllabus" Student="Y">
    <Content>&lt;ol&gt;&lt;li class="MsoNormal" style="line-height:normal;mso-list:l0 level1 lfo1;tab-stops:list 36.0pt;"&gt;&lt;strong&gt;The Universe and its scale:&lt;/strong&gt;&amp;nbsp;A tour of the Universe, its scale and contents; astronomical units&lt;o:p&gt;&lt;/o:p&gt;&lt;/li&gt;&lt;li class="MsoNormal" style="line-height:normal;mso-list:l0 level1 lfo1;tab-stops:list 36.0pt;"&gt;&lt;strong&gt;Gravitation&lt;/strong&gt;: Newton’s gravity, Kepler’s laws&lt;o:p&gt;&lt;/o:p&gt;&lt;/li&gt;&lt;li class="MsoNormal" style="line-height:normal;mso-list:l0 level1 lfo1;tab-stops:list 36.0pt;"&gt;&lt;strong&gt;Observational astronomy:&lt;/strong&gt;&amp;nbsp;the electromagnetic spectrum; blackbody radiation, the Planck, Stefan-Boltzmann and Wien laws, geometrical optics; telescopes and detectors;&amp;nbsp;&lt;o:p&gt;&lt;/o:p&gt;&lt;/li&gt;&lt;li class="MsoNormal" style="line-height:normal;mso-list:l0 level1 lfo1;tab-stops:list 36.0pt;"&gt;&lt;strong&gt;Distances:&lt;/strong&gt;&amp;nbsp;parallax measurements, standard candles&lt;o:p&gt;&lt;/o:p&gt;&lt;/li&gt;&lt;li class="MsoNormal" style="line-height:normal;mso-list:l0 level1 lfo1;tab-stops:list 36.0pt;"&gt;&lt;strong&gt;Physics of the Sun and Stars:&lt;/strong&gt;&amp;nbsp;Hertzsprung-Russell diagram; &amp;nbsp;hydrogen spectral lines and Doppler effect; Freefall and Kelvin-Helmholtz time; nucleosynthesis; basic stellar structure (hydrostatic equilibrium, equation of state); white dwarfs, neutron stars, and black holes&lt;o:p&gt;&lt;/o:p&gt;&lt;/li&gt;&lt;li class="MsoNormal" style="line-height:normal;mso-list:l0 level1 lfo1;tab-stops:list 36.0pt;"&gt;&lt;strong&gt;Galaxies:&lt;/strong&gt;&amp;nbsp; Star formation and the interstellar medium; stellar populations;&amp;nbsp;galaxy rotation curves, mass and dark matter;&amp;nbsp;&lt;o:p&gt;&lt;/o:p&gt;&lt;/li&gt;&lt;li class="MsoNormal" style="line-height:normal;mso-list:l0 level1 lfo1;tab-stops:list 36.0pt;"&gt;&lt;strong&gt;Cosmology:&lt;/strong&gt;&amp;nbsp; Hubble's Law; the age of the Universe; Evidence for the Big Bang (blackbody radiation, nucleosynthesis); dark energy and the accelerating Universe.&lt;o:p&gt;&lt;/o:p&gt;&lt;/li&gt;&lt;/ol&gt;</Content>
  </Syllabus>
  <TeachingMethods Applicant="Y" Label="Teaching and learning methods" Student="Y">
    <Content>&lt;p&gt;Two one hour, live in-person lectures per week where the core material with examples will be delivered. The lectures contain interactive elements such as mentimeter quizzes. The recordings of these lectures will be linked on the course page. The lecture slides shown during lectures will be available in pdf format. There will be written lecture summary notes available online. Links to online demonstrations and online material such as videos or animations will be. There will be weekly exercises which will be delivered via an online quiz. The weekly online quiz will be submitted weekly, then marking including written feedback will be delivered via teaching assistants and unit lead. The solutions will be discussed during weekly tutorial sessions. A Piazza discussion forum is also provided where students can ask questions with answers provided by other students and the unit lead.&amp;nbsp;&lt;/p&gt;</Content>
  </TeachingMethods>
  <AssessmentMethods Applicant="Y" Label="Assessment methods" Student="Y">
    <IntroText> </IntroText>
    <Method>
      <MethodId>0</MethodId>
      <MethodName>Other</MethodName>
      <MethodWeight>10%</MethodWeight>
    </Method>
    <Method>
      <MethodId>1</MethodId>
      <MethodName>Written exam</MethodName>
      <MethodWeight>90%</MethodWeight>
    </Method>
    <OtherDescription>&lt;p&gt;* 10%&amp;nbsp;Tutorial Work/attendance&amp;nbsp;&lt;/p&gt;</OtherDescription>
  </AssessmentMethods>
  <FeedbackMethods Applicant="Y" Label="Feedback methods" Student="Y">
    <Content>&lt;p&gt;Feedback will be offered by tutors on students&amp;rsquo; written solutions to weekly examples sheets, for which model answers will also be issued.&lt;/p&gt;</Content>
  </FeedbackMethods>
  <RequirementsList Applicant="Y" Label="Pre/co-requisites" Student="Y">
    <Requirement>
      <UnitCode></UnitCode>
      <UnitTitle></UnitTitle>
      <RequirementType></RequirementType>
      <Description></Description>
    </Requirement>
    <AdditionalRequirement></AdditionalRequirement>
  </RequirementsList>
  <AcademicPrograms Applicant="Y" Label="Academic programmes" Student="Y">
    <AcademicProgram>
      <Program></Program>
      <Plan></Plan>
      <Level></Level>
      <Requirement></Requirement>
    </AcademicProgram>
  </AcademicPrograms>
  <FreeChoice Applicant="Y" Label="Available as a free choice unit?" Student="Y">
    <Content>N</Content>
  </FreeChoice>
  <Accreditation Applicant="Y" Label="Accreditation" Student="Y">
    <Content></Content>
  </Accreditation>
  <RecommendedReading Applicant="Y" Label="Recommended reading" Student="Y">
    <Content>&lt;p class="MsoNormal" style="line-height:normal;"&gt;An introduction to modern astrophysics, Carroll, Bradley W.; Ostlie, Dale A., Pearson, 2013, ISBN: 9781292022932&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Astrophysics in a nutshell, Maoz, Dan&lt;span style="mso-tab-count:1;"&gt;&amp;nbsp;&lt;/span&gt;Princeton University Press, 2016, ISBN: 0691164797&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Astrophysics in a nutshell, Maoz, Dan, Princeton University Press, 2007, ISBN: 0691125848&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;An introduction to the Sun and stars, Green, Simon F.; Jones, Mark H.; Burnell, Jocelyn Bell; Open University, Cambridge University Press, 2004, ISBN: 0521546222&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;An introduction to galaxies and cosmology, Jones, Mark H.; Lambourne, Robert J. A., Cambridge University Press, 2004, ISBN: 0521546230&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Astronomy: a physical perspective, Kutner, Marc L., Cambridge University Press, 2003, ISBN: 0521529271&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Introduction to Astronomy and Cosmology, Morison, Ian, Wiley, 2008, ISBN: 0470033347&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Essentials of astronomy, Motz, Lloyd; Duveen, Anneta, Columbia university press, 1977, ISBN: 0231040091&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;The physical universe: an introduction to astronomy, Shu, Frank H., University Science Books, 1982, ISBN: 0935702059&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;&lt;p class="MsoNormal" style="line-height:normal;"&gt;Introductory astronomy &amp;amp; astrophysics, Zeilik, Michael; Gregory, Stephen A., Thomson, Learning, 1998, ISBN: 0030062284&lt;o:p&gt;&lt;/o:p&gt;&lt;/p&gt;</Content>
  </RecommendedReading>
  <StudyHours Applicant="Y" Label="Study hours" Student="Y">
    <IntroText> </IntroText>
    <ScheduledHours Applicant="Y" Label="Scheduled activity hours" Student="Y">
      <ActivityHours>
        <ActivityType>Assessment written exam</ActivityType>
        <Hours>1.5</Hours>
      </ActivityHours>
      <ActivityHours>
        <ActivityType>Lectures</ActivityType>
        <Hours>22</Hours>
      </ActivityHours>
      <ActivityHours>
        <ActivityType>Tutorials</ActivityType>
        <Hours>12</Hours>
      </ActivityHours>
    </ScheduledHours>
    <PlacementHours Applicant="Y" Label="Placement hours" Student="Y">
      <ActivityHours>
        <ActivityType></ActivityType>
        <Hours>0</Hours>
      </ActivityHours>
    </PlacementHours>
    <TotalHours Applicant="Y" Label="Independent study hours" Student="Y">
      <Hours>64.5</Hours>
    </TotalHours>
  </StudyHours>
  <Notes Applicant="Y" Label="Additional notes" Student="Y">
    <Content></Content>
  </Notes>
</CourseUnit>
