Infrared Astronomy in the heat of the night Michael Burton Infrared Astronomy ◊ What is the infrared ◊ Infrared Science • Imaging • Spectroscopy ◊ History and the Future ◊ Infrared Movies William Herschel “Calorific Rays” in 1800 Infrared is Heat Thermal Radiation Two views of a geyser QuickTime™ and a Sorenson Video decompressor are needed to see this picture. 1. Dust Extinction Exploring the hidden universe Galactic Centre Cygnu s 2. Thermal Radiation Detecting Cool Objects 3. Redshift Exploring the Early Universe Atmospheric Windows Infrared Windows QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. IR Observatories on the ground, in the air and in space The Horsehead Nebula Visible Near-IR Mid-IR Massive Star Formation Triffid Nebula The Galactic Centre Visible Near-IR Three Spectral Regimes Detector Technology QuickTime™ and a TIFF (LZW) decompressor are needed to see this picture. Some infrared science ◊ ◊ ◊ ◊ ◊ Solar System Star Formation Stars Disks and Planets Galaxies Venus Infrared emission vs. Visible reflection Jupiter Bright belts, volcanic Io, methane absorption Star Formation Orion Constellation Far-IR Dust Orion Nebula Near-IR Young Stars Nearby Globule Mid-IR Dust + Protostars Massive Stars ◊ Pistol Star • Most luminous star in Galaxy • ~107 L ◊ Quintuplet Cluster • Most massive star cluster in Galaxy • Max mass of a star? Dust Disks and Planets Beta Pictoris HR4796A The Galaxy Near + mid-IR Galactic Centre Red Giants + Hot Dust Far--IR Galactic Plane Zodiacal Light + Warm Dust Other Galaxies: Spiral M81 ◊ Old Stars (blue) ◊ Heated Dust (red) ◊ Hot Dust and MSF (green + knots) Global Star Formation Spiral Galaxy M51 Hidden Black Holes in the IR Infrared Spectroscopy ◊ Cooling Lines • Molecules • Fine structure lines ◊ Ices ◊ Dust Infrared Spectroscopy Water in the Solar System Hydrocarbons, Ices, Dust mineralology Cooling Lines in the ISM [OI] 63µm + [CII] 158µm Cooling Lines across the Galaxy [CII] 158µm + [NII] 205µm Water and Ices in Molecular Clouds Elements and Minerals in Red Giants and PN winds Recycling of the elements Star Formation in the Galactic Centre Hot massive stars, ionized gas, ~107 yrs Molecules in Dusty Galaxies Spiral NGC891 Starburst Arp 220 Probing the Excitation of Galaxies A potted history of IR astronomy 1800: William Herschel Discovery of IR 1870: 4th Earl of Rosse Temperature of Moon From IR on dark side 1856: Charles Piazzi IR from the Moon Thermocouple & heat 1948: Moon must be covered By fine powder IR Facilities: the early days 1961: Frank Low Germanium bolometer Cooled, in dewar Detect far-IR Change in conductivity 1967: Cooled IR telescopes in rockets AFGL IR sky survey 4+10+20µm 2363 sources in 30 mins 1960’s: Balloons carry high altitude payloads 1967: Mauna Kea Observatory established High & dry! IR Facilities Develop 1968: Leighton & Neugebauer Mt Wilson 2.2µm IR survey 5,500 sources 1974: Kuiper Airborne Observatory Rings of Uranus Water in Jupiter Early 1970’s: Most galaxies found to emit strongly in IR (M31) Mid 1970’s: Far-IR spectrometers from balloons at T = 1K CMBR IR Facilities Mature 1980’s: IR arrays 1985: IR telescope on Shuttle 1983: IRAS satellite 12+25+60+100µm 500,000 sources Vega Disk ULIRGs 1989: COBE MM + Far-IR sky CMBR IR in the 90s 1994: SPIREX at the South Pole 1996: DENIS Near-IR sky survey La Silla, Chile 1995: ESA ISO 2.5-240µm + spectroscopy 1996: MSX Military satellite 8+11+14+21µm IR Astronomy Today 1997: 2MASS All-sky 1.2 + 1.6 + 2.2µm 2001: Keck Interferometer 1997: NICMOS on HST 1-2.5µm 2004: Spitzer Space Telescope IR Astronomy Tomorrow 2007?: SOFIA - IR spectroscopy 2008?: Planck CMBR 2008?: Herschel - far-IR 2???: TPF/Darwin Other Earths?! Infrared Astronomy for Australia ◊ Siding Spring Observatory • AAT/IRIS 1-2.5µm Imager/Spectrometer • 2.3m/CASPIR 1-5µm Imager ◊ Gemini • 1-5µm NIFS + 8-25µm Michelle / TReCS ◊ Public Databases • 2MASS (1-2µm), MSX (8-21µm), GLIMPSE (48µm), IRAS (12-100µm) ◊ Antarctica • Finest ground-based sites on the Earth! Dark Cloud + HH46-47 Optical to Infrared (Spitzer) QuickTime™ and a MPEG-4 Video decompressor are needed to see this picture. Dark Globule IC1396 Visible to Infrared (Spitzer) QuickTime™ and a MPEG-4 Video decompressor are needed to see this picture. Massive Star Formation Triffid: Visible to IR (Spitzer) QuickTime™ and a decompressor are needed to see this picture. Spiral Galaxy M51 Visible to Infrared (Spitzer) QuickTime™ and a MPEG-4 Video decompressor are needed to see this picture. 2MASS 1-2µm View Galactic Centre QuickTime™ and a Sorenson Video decompressor are needed to see this picture. MSX 8-21µm view of the Galaxy PAHs along the Milky Way QuickTime™ and a Sorenson Video decompressor are needed to see this picture. Eta Carina Star Forming Complex