Dr. Steven S. Vogt

Team Discovers Second Potentially Habitable Earth-sized Exoplanet Nearby

Press Release
GJ 667C Paper (on astro-ph 2/2/12, 10:00pm PST)
GJ 667C Movie (avi)
GJ 667C Figure: Constellation View
GJ 667C Figure: Artist's Rendering by Lynette Cook
GJ 667C Figure: Phased Orbits
GJ 667C Figure: Periodograms
GJ 667C Figure: Top View

A planet-hunting team led by astronomers at UCSC and the Carnegie Institution of Washington has discovered a second earth-size planet orbiting a nearby star in the habitable zone where liquid water could exist. Findings are reported in a paper to be published in the Astrophysical Journal, which will be online at arXiv.org.

"This was expected to be a rather unlikely star to host planets. Yet there they are, around a very nearby, metal-poor example of the most common type of star in our galaxy," said Vogt, a professor of astronomy and astrophysics at UCSC. "The detection of this planet, this nearby and this soon, implies that our galaxy must be teeming with billions of potentially habitable rocky planets." [More]

APF: Automated Planet Finder Telescope

• The 2.4-meter APF, currently nearing completion atop Mt. Hamilton, is the first telescope capable of detecting rocky planets that may support life. Every night it will search robotically for these planets. [More]
• Steve is the APF P.I. and leads the team that designed and is building the Levy spectrograph, optimized for speed and radial velocity precision. Spectrograph will detect changes in a star’s velocity as small as 1 meter per second--human walking speed.
• APF Homepage
• APFCam
• DOME: Construction of APF, time-lapse movie
• Images
• APF Press Release, 8/21/10

Exoplanets: Planets Beyond our Solar System

• The ultimate goal of extrasolar planet search is to discover a solar system similar to our own with earth-like planets capable of supporting life.
• Steve's roles in Exoplanet project:
• Built Hamilton spectrometer,with which many of the first planets were found
• Re-optimized the Hamilton optics in 1994 to increase the Exoplanet's rv precision from 10 m/s to 3 m/s
• Built HIRES for Keck and incorporated Iodine cell for exoplanet work
• Principal member of the California-Carnegie Exoplanet Team from 1995-2007
• P.I. of the Automated Planet Finder facility 2001-present
• Co-leader (with Paul Butler) of the Lick-Carnegie Exoplanet Team 2007-present
• Exoplanet Press Release, 9/29/10
• Artist's images of Extrasolar Planets: Lynette Cook's illustrations
• Earthbound homepage

TMT: Thirty Meter Telescope

• TMT will be an extremely large telescope, with a 30-meter mirror comprised of 492 hexagonal-shaped segments. The spectrometer will analyze light in visible and infrared wavelengths to help astronomers answer such profound questions as "How do planets form?" and "What is the ultimate fate of our galaxy?"
• Steve completed and tendered to the TMT project a detailed design study for a Moderate-To-High-Resolution Spectrometer (MTHR) which will enable TMT to deliver the full advantage of its large aperture at first-light for high-resolution optical spectroscopy. [Read more]
• Project Manager's Reports: Status of TMT
• Spectrograph CAD rendering
• TMT homepage

HIRES: High Resolution Echelle Spectrograph

• HIRES is a high resolution optical spectrometer mounted permanently on the Keck 10-meter telescope on Mauna Kea, Hawaii.
• Steve designed and built the Keck HIRES from 1987 - 1993.
• Spectrograph illustration
• 2004 CCD Upgrade
• Keck Observatory
• HIRES homepage

Hamilton Echelle Spectrograph

• The Hamilton Spectrograph, designed by Steve Vogt and installed at the coudé focus of Lick Observatory's Shane telescope in 1987, is still frequently used to observe distant objects.
• Steve roles in Hamilton Spectrograph Project:
• P.I. of project
• Originated the concept
• Designed the optics with Harland Epps
• Oversaw all detailed mechanical, electronic, and optical design and fabrication
• Installed and commissioned spectrograph
• Read Steve's paper on the Hamilton Spectrograph and the philosophy behind its design
• Public information about the Hamilton Spectrograph